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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Cell. Neurosci.</journal-id>
<journal-title>Frontiers in Cellular Neuroscience</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Cell. Neurosci.</abbrev-journal-title>
<issn pub-type="epub">1662-5102</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.3389/fncel.2017.00301</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Neuroscience</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Non-aggregated A&#x03B2;25-35 Upregulates Primary Astrocyte Proliferation <italic>In Vitro</italic></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name><surname>Ohki</surname> <given-names>Elise C.</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Langan</surname> <given-names>Thomas J.</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
<xref ref-type="aff" rid="aff3"><sup>3</sup></xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Rodgers</surname> <given-names>Kyla R.</given-names></name>
<xref ref-type="aff" rid="aff4"><sup>4</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/449792/overview"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name><surname>Chou</surname> <given-names>Richard C.</given-names></name>
<xref ref-type="aff" rid="aff4"><sup>4</sup></xref>
<xref ref-type="aff" rid="aff5"><sup>5</sup></xref>
<xref ref-type="author-notes" rid="fn001"><sup>&#x002A;</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/435698/overview"/>
</contrib>
</contrib-group>
<aff id="aff1"><sup>1</sup><institution>Department of Interdisciplinary Natural Sciences, Roswell Park Cancer Institute, State University of New York at Buffalo</institution>, <addr-line>Buffalo, NY</addr-line>, <country>United States</country></aff>
<aff id="aff2"><sup>2</sup><institution>Departments of Neurology, Pediatrics, and Physiology and Biophysics, Jacobs School of Medicine and Biomedical Sciences, State University of New York at Buffalo</institution>, <addr-line>Buffalo, NY</addr-line>, <country>United States</country></aff>
<aff id="aff3"><sup>3</sup><institution>Hunter James Kelly Research Institute, New York State Center of Excellence Bioinformatics &#x0026; Life Sciences</institution>, <addr-line>Buffalo, NY</addr-line>, <country>United States</country></aff>
<aff id="aff4"><sup>4</sup><institution>Department of Medicine, Geisel School of Medicine at Dartmouth</institution>, <addr-line>Lebanon, NH</addr-line>, <country>United States</country></aff>
<aff id="aff5"><sup>5</sup><institution>Section of Rheumatology, Department of Medicine, Dartmouth-Hitchcock Medical Center</institution>, <addr-line>Lebanon, NH</addr-line>, <country>United States</country></aff>
<author-notes>
<fn fn-type="edited-by"><p>Edited by: <italic>Juan Andr&#x00E9;s Orellana, Pontificia Universidad Cat&#x00F3;lica de Chile, Chile</italic></p></fn>
<fn fn-type="edited-by"><p>Reviewed by: <italic>Markel Olabarria, Columbia University, United States; Rodrigo A. Cunha, University of Coimbra, Portugal</italic></p></fn>
<fn fn-type="corresp" id="fn001"><p>&#x002A;Correspondence: <italic>Richard C. Chou, <email>richard.c.chou@hitchcock.org</email></italic></p></fn>
</author-notes>
<pub-date pub-type="epub">
<day>26</day>
<month>09</month>
<year>2017</year>
</pub-date>
<pub-date pub-type="collection">
<year>2017</year>
</pub-date>
<volume>11</volume>
<elocation-id>301</elocation-id>
<history>
<date date-type="received">
<day>11</day>
<month>05</month>
<year>2017</year>
</date>
<date date-type="accepted">
<day>11</day>
<month>09</month>
<year>2017</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#x00A9; 2017 Ohki, Langan, Rodgers and Chou.</copyright-statement>
<copyright-year>2017</copyright-year>
<copyright-holder>Ohki, Langan, Rodgers and Chou</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/"><p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p></license>
</permissions>
<abstract>
<p>Amyloid beta (A&#x03B2;) is a peptide cleaved from amyloid precursor protein that contributes to the formation of senile plaques in Alzheimer&#x2019;s disease (AD). The relationship between A&#x03B2; and astrocyte proliferation in AD remains controversial. Despite pathological findings of increased astrocytic mitosis in AD brains, <italic>in vitro</italic> studies show an inhibitory effect of A&#x03B2; on astrocyte proliferation. In this study, we determined the effect of an active fragment of A&#x03B2; (A&#x03B2;<sub>25-35</sub>) on the cell cycle progression of primary rat astrocytes. We found that A&#x03B2;<sub>25-35</sub> (0.3&#x2013;1.0 &#x03BC;g/ml) enhanced astrocyte proliferation <italic>in vitro</italic> in a time- and concentration-dependent manner. Increased DNA synthesis by A&#x03B2;<sub>25-35</sub> was observed during the S phase of the astrocyte cell cycle, as indicated by proliferation kinetics and bromodeoxyuridine immunocytochemical staining. Aggregation of A&#x03B2;<sub>25-35</sub> abolished the upregulatory effect of A&#x03B2; on astrocyte proliferation. Further examination indicated that A&#x03B2;<sub>25-35</sub> affected astrocyte proliferation during early or mid-G<sub>1</sub> phase but had no effect on DNA synthesis at the peak of S phase. These results provide insight into the relationship between A&#x03B2;<sub>25-35</sub> and astrocyte cell cycling in AD.</p>
</abstract>
<kwd-group>
<kwd>astrocyte</kwd>
<kwd>amyloid beta</kwd>
<kwd>cell cycle</kwd>
<kwd>primary cultures</kwd>
<kwd>Alzheimer&#x2019;s disease</kwd>
</kwd-group>
<counts>
<fig-count count="5"/>
<table-count count="2"/>
<equation-count count="0"/>
<ref-count count="71"/>
<page-count count="10"/>
<word-count count="0"/>
</counts>
</article-meta>
</front>
<body>
<sec><title>Introduction</title>
<p>Alzheimer&#x2019;s disease (AD), the most common form of neurodegenerative disease (<xref ref-type="bibr" rid="B5">Alzheimer&#x2019;s Association, 2015</xref>), is characterized by two pathological hallmarks: senile plaques composed of amyloid beta (A&#x03B2;) and neurofibrillary tangles made up of hyperphosphorylated tau (<xref ref-type="bibr" rid="B58">Scheltens et al., 2016</xref>). Deposition of A&#x03B2; fibrils is an early finding in AD brains (<xref ref-type="bibr" rid="B53">Roth et al., 1966</xref>; <xref ref-type="bibr" rid="B46">Pike et al., 1995a</xref>; <xref ref-type="bibr" rid="B49">Rama Rao and Kielian, 2015</xref>). A&#x03B2; is a peptide that is proteolytically cleaved from transmembrane amyloid precursor protein (APP) by alpha, beta, or gamma secretases and can vary in length (<xref ref-type="bibr" rid="B32">LaFerla et al., 2007</xref>; <xref ref-type="bibr" rid="B13">Chow et al., 2010</xref>). Mutations in either APP or presenilins, which are the catalytic subunits of the gamma secretase complex, increase the risk for AD, possibly by elevating the production of abnormal APP cleavage products that are more prone to forming pathogenic fibrils (<xref ref-type="bibr" rid="B25">Iwatsubo et al., 1994</xref>, <xref ref-type="bibr" rid="B24">1995</xref>; <xref ref-type="bibr" rid="B20">Gu and Guo, 2013</xref>). Several different A&#x03B2; fragments alter the functions of neurons and glia, including A&#x03B2;<sub>25-35</sub> (<xref ref-type="bibr" rid="B23">Iversen et al., 1995</xref>; <xref ref-type="bibr" rid="B40">Millucci et al., 2010</xref>; <xref ref-type="bibr" rid="B1">Abeti et al., 2011</xref>; <xref ref-type="bibr" rid="B14">Dal Pra et al., 2011</xref>), A&#x03B2;<sub>1-42</sub> (<xref ref-type="bibr" rid="B23">Iversen et al., 1995</xref>; <xref ref-type="bibr" rid="B14">Dal Pra et al., 2011</xref>; <xref ref-type="bibr" rid="B8">Blennow et al., 2015</xref>), A&#x03B2;<sub>22-35</sub> (<xref ref-type="bibr" rid="B67">Takadera et al., 1993</xref>; <xref ref-type="bibr" rid="B23">Iversen et al., 1995</xref>), and A&#x03B2;<sub>12-28</sub> (<xref ref-type="bibr" rid="B23">Iversen et al., 1995</xref>; <xref ref-type="bibr" rid="B19">Giulian et al., 1996</xref>). Each of these species has different propensities for forming aggregates and senile plaques (<xref ref-type="bibr" rid="B31">Kummer and Heneka, 2014</xref>). Among these A&#x03B2;<sub>25-35</sub> was also shown to induce the production of A&#x03B2;<sub>1-42</sub> in cultured human astrocytes (<xref ref-type="bibr" rid="B14">Dal Pra et al., 2011</xref>). Although A&#x03B2; is believed to be critical for the development of AD, the biology of different peptide species and their aggregates, as well as the mechanisms by which they drive pathogenesis remain largely unknown (<xref ref-type="bibr" rid="B16">De Strooper and Karran, 2016</xref>).</p>
<p>Interestingly, amyloid deposits and senile plaques are surrounded by reactive astrocytes (<xref ref-type="bibr" rid="B46">Pike et al., 1995a</xref>; <xref ref-type="bibr" rid="B49">Rama Rao and Kielian, 2015</xref>), a phenomenon noted by Alzheimer himself in his initial pathological analysis and recently confirmed by others (<xref ref-type="bibr" rid="B4">Alzheimer et al., 1995</xref>; <xref ref-type="bibr" rid="B57">Santillo et al., 2011</xref>). Although remaining in a state of quiescence under normal circumstances, mammalian astrocytes play critical roles in the biochemical and physiological functions of the central nervous system (<xref ref-type="bibr" rid="B33">Langan, 1993</xref>), including shaping synaptic transmission (<xref ref-type="bibr" rid="B41">Murphy-Royal et al., 2015</xref>), regulating cerebral blood flow (<xref ref-type="bibr" rid="B71">Zonta et al., 2003</xref>), and maintaining proper levels of extracellular ions and neurotransmitters (<xref ref-type="bibr" rid="B64">Simard and Nedergaard, 2004</xref>; <xref ref-type="bibr" rid="B43">Olsen et al., 2015</xref>). However, in AD and other pathological conditions, astrocytes undergo metabolic and phenotypic transformations, re-entering the cell cycle and actively proliferating, a state known as reactive astrogliosis (<xref ref-type="bibr" rid="B6">Amaducci et al., 1981</xref>; <xref ref-type="bibr" rid="B44">Pekny et al., 2016</xref>; <xref ref-type="bibr" rid="B50">Rodriguez-Arellano et al., 2016</xref>). Reactivation of astrocytes is thought to be a crucial early step in the pathogenesis of AD, and prevention of astrogliosis has been proposed as a potential therapeutic strategy (<xref ref-type="bibr" rid="B45">Pekny et al., 2014</xref>, <xref ref-type="bibr" rid="B44">2016</xref>; <xref ref-type="bibr" rid="B60">Scholl et al., 2015</xref>; <xref ref-type="bibr" rid="B50">Rodriguez-Arellano et al., 2016</xref>). The mechanisms underlying cell-cycle re-entry in astrocytes and the relationship between different A&#x03B2; species, aggregation states, and reactive astrogliosis remain a matter of intense debate, and further investigation is necessary before novel therapeutic strategies can be proposed (<xref ref-type="bibr" rid="B27">Jordan-Sciutto et al., 2002</xref>; <xref ref-type="bibr" rid="B18">Gartner et al., 2003</xref>; <xref ref-type="bibr" rid="B69">Yang et al., 2006</xref>).</p>
<p>The goal of the present study was to gain a better understanding of the functional relationship between A&#x03B2; and proliferation of astrocytes. We hypothesized that soluble A&#x03B2;, but not aggregated (agA&#x03B2;), promotes astrocyte reactivation regardless of cell-cycle phase. To test this hypothesis, we treated serum-deprived and non-serum-deprived rat astrocytes with A&#x03B2;<sub>25-35</sub> and measured their rates of proliferation after varying lengths of time <italic>in vitro</italic>. We further investigated if aggregation of soluble A&#x03B2;<sub>25-35</sub> alters its effects on astrocytes. Our results provide insight into the functional roles of A&#x03B2;<sub>25-35</sub>, as well as results of its aggregation, in reactive astrocytosis.</p>
</sec>
<sec id="s1" sec-type="materials|methods">
<title>Materials and Methods</title>
<sec><title>Primary Astrocyte Culture</title>
<p>All experimental procedures were approved by the Institutional Animal Care and Use Committee (IACUC) at the SUNY at Buffalo, and all experiments were carried out in accordance with the approved procedures. Newborn pups were purchased from Harlan Sprague-Dawley and housed briefly in the Animal Research Center, SUNY at Buffalo. The cerebral cortices of newborn (&#x003C;48 h) Sprague-Dawley rat pups (Harlan Sprague Dawley, Indianapolis, IN, United States) were harvested and mechanically dissociated. Astrocytes were isolated by filtration through nylon mesh with 20 &#x03BC;m pore size to remove tissue debris (<xref ref-type="bibr" rid="B37">Langan and Slater, 1992</xref>; <xref ref-type="bibr" rid="B34">Langan and Chou, 2011</xref>). Primary astrocyte cultures were maintained in 10% fetal bovine serum (Hyclone, Logan, UT, United States) and 1% penicillin&#x2013;streptomycin (v/v; Sigma, St. Louis, MO, United States) in Dulbecco&#x2019;s modified Eagle&#x2019;s medium (DMEM) (Gibco/Life Technologies, Inc., Grand Island, NY, United States) at 37&#x00B0;C in a CO<sub>2</sub> incubator (5% CO<sub>2</sub>/95% humidified air) until <italic>in vitro</italic> studies. A previous study shows that the initial astrocyte cultures generated by this method are of &#x2265;95% purity (<xref ref-type="bibr" rid="B34">Langan and Chou, 2011</xref>; <xref ref-type="bibr" rid="B35">Langan et al., 2017</xref>).</p>
</sec>
<sec><title>Astrocyte Subculture and <italic>In Vitro</italic> Stimulation</title>
<sec><title>Non-serum-Deprivation Experiments</title>
<p>Primary astrocytes were harvested by trypsinization and passaged into 6-well plates at a concentration of 1 &#x00D7; 10<sup>4</sup> cells/cm<sup>2</sup> in 10% bovine calf serum (BCS; Hyclone)/DMEM (v/v). After an initial 2-h incubation at 37&#x00B0;C in 5% CO<sub>2</sub>/95% humidified air, the medium was removed, and cell cultures were washed once with phosphate-buffered saline (PBS, pH 7.4) to remove cell debris and non-adherent cells; 3 ml of 10% BCS/DMEM was then added to adherent cells. Astrocytes were allowed to proliferate at 37&#x00B0;C in 5% CO<sub>2</sub>/95% humidified air for 48 h. At the end of incubation, the supernatant was replaced with 2 ml fresh 10% BCS/DMEM in the presence of varying concentrations of agA&#x03B2;<sub>25-35</sub> (in PBS, pH 7.4), freshly prepared non-agA&#x03B2;<sub>25-35</sub> (in PBS, pH 7.4), or control peptide (CP; Cal-Biochem, La Jolla, CA, United States) (in PBS, pH 7.4), which was the A&#x03B2; fragment of interest with the amino acids in reverse order (i.e., A&#x03B2;<sub>35-25</sub>). This step represented the start of the experiment (i.e., <italic>T</italic><sub>0</sub>).</p>
</sec>
<sec><title>Serum-Deprivation Experiments</title>
<p>Astrocytes were passaged into 6-well plates at a concentration of 1 &#x00D7; 10<sup>4</sup> cells/cm<sup>2</sup> in 10% BCS/DMEM. Cells were then allowed to grow to 30&#x2013;50% confluence in 10% BCS/DMEM at 37&#x00B0;C in 5% CO<sub>2</sub>/95% humidified air. At the end of incubation, the medium was removed, and cells were rinsed with PBS (pH 7.4). Cells were then overlaid with 3 ml 0.1% BCS/DMEM and incubated at 37&#x00B0;C in 5% CO<sub>2</sub>/95% humidified air for 48 h, such that by the end of the incubation period, 85&#x2013;90% of cells entered cell-cycle arrest (<xref ref-type="bibr" rid="B36">Langan and Slater, 1991</xref>; <xref ref-type="bibr" rid="B12">Chou and Langan, 2003</xref>; <xref ref-type="bibr" rid="B34">Langan and Chou, 2011</xref>; <xref ref-type="bibr" rid="B35">Langan et al., 2017</xref>). At the end of the serum-deprivation process, the medium was replaced with 2 ml 10% BCS/DMEM. This serum up-shift allowed astrocytes to re-enter the cell cycle in a first-order manner and represented the start of the cell-cycle entry experiment (i.e., <italic>T</italic><sub>0</sub>) (<xref ref-type="bibr" rid="B38">Langan and Volpe, 1987</xref>; <xref ref-type="bibr" rid="B29">Kniss and Burry, 1988</xref>; <xref ref-type="bibr" rid="B12">Chou and Langan, 2003</xref>; <xref ref-type="bibr" rid="B34">Langan and Chou, 2011</xref>; <xref ref-type="bibr" rid="B35">Langan et al., 2017</xref>). Varying concentrations of agA&#x03B2;<sub>25-35</sub>, non-aggregated (freshly prepared) A&#x03B2;<sub>25-35</sub>, or CP were added to the cultures concurrently with the medium, allowing astrocytes to re-enter the cell cycle under defined experimental conditions.</p>
</sec>
</sec>
<sec><title>A&#x03B2;<sub>25-35</sub> and Its Aggregation</title>
<p>The A&#x03B2;<sub>25-35</sub> peptide is a truncated product of A&#x03B2; that was shown to be physiologically active, and was widely published in articles using rat models of AD (<xref ref-type="bibr" rid="B65">Soto et al., 1998</xref>; <xref ref-type="bibr" rid="B7">Arif et al., 2009</xref>; <xref ref-type="bibr" rid="B17">Fedotova et al., 2016</xref>; <xref ref-type="bibr" rid="B42">Nell et al., 2016</xref>; <xref ref-type="bibr" rid="B66">Soultanov et al., 2016</xref>). Others have shown that the effects of A&#x03B2;<sub>25-35</sub> on different cellular functions in both astrocytes and neurons are similar to those of A&#x03B2;<sub>1-42</sub> (<xref ref-type="bibr" rid="B11">Chiarini et al., 2010</xref>; <xref ref-type="bibr" rid="B28">Kaminsky et al., 2010</xref>); additionally, although its physiologic role remains unclear, histopathological studies have shown that A&#x03B2;<sub>25-35</sub> is present in senile plaques of Alzheimer&#x2019;s brains (<xref ref-type="bibr" rid="B30">Kubo et al., 2003</xref>). For these reasons, A&#x03B2;<sub>25-35</sub> is the focus of the present studies using rat astrocytes. Quantitative analysis of A&#x03B2;<sub>25-35</sub> aggregation by sedimentation assay was performed according to an established procedure (<xref ref-type="bibr" rid="B47">Pike et al., 1994</xref>, <xref ref-type="bibr" rid="B48">1995b</xref>). In brief, the lysine residues in the non-agA&#x03B2;<sub>25-35</sub> fragment react with the fluorescent marker fluorescamine (FLCN; Molecular Probes, Inc., Eugene, OR, United States). Aggregation of the A&#x03B2;<sub>25-35</sub> fragments is measured by a decrease in the number of lysine residues available to bind to FLCN, resulting in a reduction in fluorescence intensity proportional to the extent of aggregation. Different concentrations of A&#x03B2;<sub>25-35</sub> and CP were solubilized in 1 ml PBS (pH 7.4) at room temperature (RT) for 2 or 48 h. Aliquots of the FLCN solution in acetonitrile were added to each set of samples to achieve a 1:1 mol/ml ratio of peptide to FLCN. Following the addition of FLCN, half of the samples were measured for FLCN fluorescence without centrifugation, and half were centrifuged at 100,000 &#x00D7; <italic>g</italic> for 1 h, and the supernatant was used to measure FLCN fluorescence (<xref ref-type="bibr" rid="B48">Pike et al., 1995b</xref>). Fluorescence was measured at 478 nm by exciting the peptide at 383 nm with a fluorescence (LS-5) spectrophotometer (Perkin-Elmer, Norwalk, CT, United States) (<xref ref-type="bibr" rid="B15">De Bernardo et al., 1974</xref>; <xref ref-type="bibr" rid="B3">Alavi et al., 2013</xref>).</p>
</sec>
<sec><title>Cell Proliferation Assays</title>
<sec><title><sup>3</sup>H-Thymidine Incorporation Assay</title>
<p>The incorporation of tritiated [methyl-<sup>3</sup>H]-thymidine into primary astrocytes was used to quantify cell proliferation according to established procedures (<xref ref-type="bibr" rid="B38">Langan and Volpe, 1987</xref>; <xref ref-type="bibr" rid="B37">Langan and Slater, 1992</xref>; <xref ref-type="bibr" rid="B12">Chou and Langan, 2003</xref>; <xref ref-type="bibr" rid="B34">Langan and Chou, 2011</xref>; <xref ref-type="bibr" rid="B35">Langan et al., 2017</xref>). Radio-labeled [methyl-<sup>3</sup>H]-thymidine (25 Ci/mmol; Amersham, Arlington Heights, IL, United States) was added to each well 1 h prior to the termination of the experiment at a final activity of 1.0 &#x03BC;Ci/ml (37&#x00B0;C, 5% CO<sub>2</sub>/95% humidified air). At the end of the incubation, cultures were washed with 2 ml Tris&#x2013;EDTA buffer (pH 7.4) twice to remove any excess <sup>3</sup>H-thymidine. DNA and total cellular protein were extracted using the trichloroacetic acid precipitation method (<xref ref-type="bibr" rid="B38">Langan and Volpe, 1987</xref>; <xref ref-type="bibr" rid="B37">Langan and Slater, 1992</xref>). Cell proliferation was measured as the incorporation of radioactivity per microgram of protein present in the acid-precipitated portion (cpm/&#x03BC;g protein). Tritium was quantified in the samples with a beta counter (LKB Wallac, Gaithersburg, MD, United States) for 10 min using an Ecoscint-A liquid scintillation cocktail (National Diagnostics, Manville, NJ, United States), and the total cellular protein in the samples was determined by Bradford assay (BioRad, Hercules, CA, United states) using a microplate reader (model 3550-UV; BioRad, Hercules, CA, United states) at a wavelength of 595 nm.</p>
</sec>
<sec><title>BrdU Incorporation Assay</title>
<p>The number of cells undergoing active DNA synthesis was quantified by immunocytochemical staining for bromodeoxyuridine (BrdU) (Sigma) (<xref ref-type="bibr" rid="B70">Yong et al., 1988</xref>; <xref ref-type="bibr" rid="B36">Langan and Slater, 1991</xref>). Primary astrocyte cultures were passaged onto 4.9 mm<sup>2</sup> glass cover slips coated with poly-lysine (Sigma) in 12-well plates, grown to 30&#x2013;50% confluency, and rendered into cell cycle arrest by serum deprivation as described above. Serum-deprived astrocytes were then allowed to re-enter the cell cycle under experimental conditions. To identify cells undergoing active DNA synthesis, BrdU was added to cell cultures at a final concentration of 15 &#x03BC;M for a period of 2.5 h prior to the termination of experiments. At the end of incubation, the cover slips were removed and rinsed with PBS (pH 7.4) followed by fixation with 4% paraformaldehyde (PFA; Sigma) in PBS (pH 7.4) for 10 min at RT. After fixation, the 4% PFA was aspirated, and cells were washed twice with PBS (pH 7.4). Fixed cells were then treated with 2 M HCl (10 min, RT) to permeabilize the nuclear membrane. The HCl was removed, and cells were again washed twice with PBS (pH 7.4) followed by incubation with 0.1 M NaB<sub>4</sub>O<sub>7</sub> to neutralize the HCl (10 min, RT). After acid neutralization, the NaB<sub>4</sub>O<sub>7</sub> was removed, and cells were washed three times with PBS (pH 7.4). Next, cells were blocked with 5% bovine serum albumin in PBS (20 min, RT). Monoclonal antibody for BrdU (Sigma) was added at a dilution of 1:200 for 1 h at RT followed by the addition of goat anti-rat rhodamine-labeled secondary antibody (Sigma) at a dilution of 1:200 for 30 min. The percent of BrdU+ nuclei was calculated based on the cell count in each of the randomly selected high powered fields using a phase-fluorescent microscope (<xref ref-type="bibr" rid="B36">Langan and Slater, 1991</xref>; <xref ref-type="bibr" rid="B39">Li et al., 1996</xref>).</p>
</sec>
</sec>
<sec><title>Cell Viability</title>
<p>In parallel to the cell proliferation assays, an identical set of cells was subcultured and treated as described above for each set of experiments. At the end of each time point, cells were harvested by trypsinization, centrifuged, and resuspended in PBS. A 0.4% trypan blue solution (Sigma) was added to the cell suspension in a 1:1 v/v ratio. A manual cell count was performed using a hemocytometer.</p>
</sec>
<sec><title>Statistical Analysis</title>
<p>All experiments were repeated at least three times, and all conditions were performed in triplicate. Data were expressed as mean &#x00B1; standard error of the mean (SEM) and analyzed using Student&#x2019;s <italic>t</italic>-tests for unpaired comparisons and one-way ANOVA for multiple group comparisons. Statistical significance was defined as <italic>p</italic> &#x003C; 0.05.</p>
</sec>
</sec>
<sec><title>Results</title>
<sec><title>A&#x03B2;<sub>25-35</sub> Upregulates Proliferation of Non-serum-Deprived Astrocytes in a Time- and Concentration-Dependent Manner</title>
<p>We first examined the effect of A&#x03B2;<sub>25-35</sub> on astrocyte proliferation by measuring DNA synthesis of non-serum-deprived primary astrocytes treated with freshly prepared and graded concentrations of A&#x03B2;<sub>25-35</sub> (0.01&#x2013;3.0 &#x03BC;g/ml). Astrocytes proliferated in an exponential-like manner over a 48-h period, with a lag phase in the initial 24 h, a log phase in the next 12 h (24&#x2013;36 h), and a slowed rate of proliferation in the last 12 h tested (36&#x2013;48 h). We found that A&#x03B2;<sub>25-35</sub> increased the rate of DNA synthesis in primary astrocytes in a time- and concentration-dependent manner (<bold>Figure <xref ref-type="fig" rid="F1">1A</xref></bold>). At a concentration of 0.3 &#x03BC;g/ml, A&#x03B2;<sub>25-35</sub> only caused a significant increase in DNA synthesis after 48 h of incubation compared with control. The greatest effect on astrocyte proliferation was obtained using a concentration of 1.0 &#x03BC;g/ml A&#x03B2;<sub>25-35</sub>, which caused significant increases in DNA synthesis after 24, 36, and 48 h of incubation. A further increase in the concentration of A&#x03B2;<sub>25-35</sub> to 3.0 &#x03BC;g/ml did not upregulate the rate of astrocyte proliferation at any time point, which therefore followed a classical concentration-effect response (<bold>Figure <xref ref-type="fig" rid="F1">1A</xref></bold>). Based on these findings, we utilized A&#x03B2;<sub>25-35</sub> at a concentration of 1.0 &#x03BC;g/ml in subsequent experiments.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption><p>The effect and specificity of A&#x03B2;<sub>25-35</sub> on proliferation of non-serum-deprived primary astrocytes. <bold>(A)</bold> Subcultured astrocytes were incubated with graded concentrations of freshly prepared and solubilized A&#x03B2;<sub>25-35</sub> or control. <sup>3</sup>H-thymidine was added to cultures 1 h prior to termination. Cultures were terminated every 12 h and processed for <sup>3</sup>H-thymidine uptake to measure rate of DNA synthesis. <bold>(B)</bold> Subcultured astrocytes were incubated with freshly prepared A&#x03B2;<sub>25-35</sub> or CP at various concentrations for 36 or 48 h. Rate of DNA synthesis was measured using <sup>3</sup>H-thymidine incorporation assay. <sup>&#x2217;</sup><italic>p</italic> &#x003C; 0.05; <sup>&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.02; <sup>&#x2217;&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.001 (results were average values of three representative experiments).</p></caption>
<graphic xlink:href="fncel-11-00301-g001.tif"/>
</fig>
<p>We next examined the specificity of the response to A&#x03B2;<sub>25-35</sub> by treating primary astrocytes with either A&#x03B2;<sub>25-35</sub> or CP consisting of the reversed amino acid sequence (i.e., A&#x03B2;<sub>35-25</sub>) at varying concentrations for 36 or 48 h. CP did not upregulate DNA synthesis in primary astrocyte cultures compared with control at either time point or either concentration tested (<bold>Figure <xref ref-type="fig" rid="F1">1B</xref></bold>), supporting the notion that the increased proliferation of astrocytes in response to A&#x03B2;<sub>25-35</sub> depends on its amino acid sequence.</p>
</sec>
<sec><title>A&#x03B2;<sub>25-35</sub> Upregulates DNA Synthesis During S Phase in Serum-Deprived Primary Astrocytes</title>
<p>We next addressed whether A&#x03B2;<sub>25-35</sub> affects cell-cycle kinetics of astrocytes <italic>in vitro</italic>. Astrocytes were first subcultured in serum-deprived medium that rendered cell-cycle arrest. Astrocytes were then exposed to serum up-shift (<xref ref-type="bibr" rid="B34">Langan and Chou, 2011</xref>; <xref ref-type="bibr" rid="B35">Langan et al., 2017</xref>), resulting in re-entry into the cell cycle with highly replicable kinetics (<bold>Figure <xref ref-type="fig" rid="F2">2</xref></bold>). Consistent with previous studies (<xref ref-type="bibr" rid="B37">Langan and Slater, 1992</xref>; <xref ref-type="bibr" rid="B33">Langan, 1993</xref>), following serum up-shift, astrocytes remained in G<sub>1</sub> phase for 12 h and then entered the S phase for the next 12 h, as shown by a first-order increase in DNA synthesis (<bold>Figure <xref ref-type="fig" rid="F2">2</xref></bold>). When astrocytes re-entered the cell cycle in the presence of A&#x03B2;<sub>25-35</sub> (1 &#x03BC;g/ml), the rate of proliferation was significantly upregulated compared with CP-treated astrocytes (<bold>Figure <xref ref-type="fig" rid="F2">2</xref></bold>). A&#x03B2;<sub>25-35</sub> did not impact the length of G<sub>1</sub> or increase the rate of proliferation of astrocytes during this time, suggesting that the effect of A&#x03B2;<sub>25-35</sub> on astrocytes is restricted to S phase. Additionally, altered proliferation in serum-deprived astrocytes was specifically mediated by A&#x03B2;<sub>25-35</sub>, as CP did not significantly impact DNA synthesis compared with control (<bold>Figure <xref ref-type="fig" rid="F2">2</xref></bold>).</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption><p>The effect of A&#x03B2;<sub>25-35</sub> on proliferation of serum-deprived primary astrocytes. Newborn astrocytes were rendered into G<sub>0</sub> phase by serum deprivation and then allowed to re-enter the cell cycle via serum up-shift in the presence of freshly prepared A&#x03B2;<sub>25-35</sub> (1.0 &#x03BC;g/ml) or CP (1.0 &#x03BC;g/ml). <sup>3</sup>H-thymidine incorporation assay was performed to measure rate of DNA synthesis. <sup>&#x2217;</sup><italic>p</italic> &#x003C; 0.05; <sup>&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.02; <sup>&#x2217;&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.001 (results were average values of three representative experiments).</p></caption>
<graphic xlink:href="fncel-11-00301-g002.tif"/>
</fig>
<p>We confirmed these findings using immunocytochemical staining for BrdU (<bold>Figure <xref ref-type="fig" rid="F3">3</xref></bold> and <bold>Table <xref ref-type="table" rid="T1">1</xref></bold>) and quantifying the percent of BrdU+ cells at <italic>T</italic><sub>0</sub> and <italic>T</italic><sub>24</sub> in the presence or absence of A&#x03B2;<sub>25-35</sub> (1 &#x03BC;g/ml). Following 48 h of serum deprivation (i.e., <italic>T</italic><sub>0</sub>), more than 81% of cells were in a state of quiescence (<bold>Figure <xref ref-type="fig" rid="F3">3</xref></bold> and <bold>Table <xref ref-type="table" rid="T1">1</xref></bold>). At <italic>T</italic><sub>24</sub>, the peak of S phase, about 65% of the cells were BrdU+, indicating that they had re-entered the cell cycle and undergone active proliferation (<bold>Figure <xref ref-type="fig" rid="F3">3</xref></bold> and <bold>Table <xref ref-type="table" rid="T1">1</xref></bold>). In the presence of A&#x03B2;<sub>25-35</sub>, significantly more astrocytes re-entered the cell cycle, as indicated by BrdU+ staining (<bold>Figure <xref ref-type="fig" rid="F3">3</xref></bold> and <bold>Table <xref ref-type="table" rid="T1">1</xref></bold>). This increase in the percentage of BrdU+ cells was specific to A&#x03B2;<sub>25-35</sub> treatment, as there was no significant change in the percentage of BrdU+ cells after 24 h of incubation with CP (<bold>Figure <xref ref-type="fig" rid="F3">3</xref></bold> and <bold>Table <xref ref-type="table" rid="T1">1</xref></bold>) compared to control.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption><p>The effect of A&#x03B2;<sub>25-35</sub> on BrdU incorporation in serum-deprived primary astrocytes. Newborn astrocytes were serum deprived for 48 h, resulting in cell cycle arrest, as demonstrated by low BrdU+ cell count (<bold>A</bold>; 18.38 &#x00B1; 0.02%, <italic>n</italic> = 9, total cell count = 102). Following serum deprivation, cells were stimulated to re-enter the cell cycle in the presence of either freshly prepared A&#x03B2;<sub>25-35</sub> (1.0 &#x03BC;g/ml) or CP (1.0 &#x03BC;g/ml). BrdU was added to the cultures 2.5 h prior to termination. After 24 h of incubation, samples were processed for immunocytochemical staining of BrdU. There was no significant difference in the number of BrdU+ cells between the control (<bold>B</bold>; 65.42 &#x00B1; 0.02%, <italic>n</italic> = 11, total cell count = 104) and CP-treated astrocytes (<bold>D</bold>; 62.44 &#x00B1; 0.02%, <italic>n</italic> = 11, total cell count = 100). Significantly more A&#x03B2;<sub>25-35</sub>-treated astrocytes were BrdU+ (<bold>C</bold>; 87.35 &#x00B1; 0.02%; <italic>n</italic> = 11, total cell count = 102, <italic>p</italic> &#x003C; 0.001) compared to controls. Images were taken with fluorescence microscopy.</p></caption>
<graphic xlink:href="fncel-11-00301-g003.tif"/>
</fig>
<table-wrap position="float" id="T1">
<label>Table 1</label>
<caption><p>Percent of BrdU+ astrocytes in response to various treatments for 24 h.</p></caption>
<table cellspacing="5" cellpadding="5" frame="hsides" rules="groups">
<thead>
<tr>
<th valign="top" align="left">Treatment</th>
<th valign="top" align="center">Time point (hour)</th>
<th valign="top" align="center">Mean &#x00B1; SEM (%)</th>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left">Control</td>
<td valign="top" align="center">0</td>
<td valign="top" align="center">18.38 &#x00B1; 0.02</td>
</tr>
<tr>
<td valign="top" align="left"></td>
<td valign="top" align="center">24</td>
<td valign="top" align="center">65.42 &#x00B1; 0.02</td>
</tr>
<tr>
<td valign="top" align="left">A&#x03B2;<sub>25-35</sub></td>
<td valign="top" align="center">24</td>
<td valign="top" align="center">87.35 &#x00B1; 0.02<sup>&#x2217;</sup></td>
</tr>
<tr>
<td valign="top" align="left">CP</td>
<td valign="top" align="center">24</td>
<td valign="top" align="center">62.44 &#x00B1; 0.02</td>
</tr>
<tr>
<td valign="top" align="left"></td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<attrib><italic><sup>&#x2217;</sup><italic>p</italic> &#x003C; 0.005.</italic></attrib>
</table-wrap-foot>
</table-wrap>
</sec>
<sec><title>Aggregation of A&#x03B2;<sub>25-35</sub> Impairs Its Effect on Proliferation Rate in Non-serum-Deprived Astrocytes</title>
<p>In order to generate agA&#x03B2;<sub>25-35</sub>, we allowed graded concentrations of A&#x03B2;<sub>25-35</sub> to aggregate for 2 or 48 h; aggregation was confirmed by measuring FLCN incorporation. Aggregation was compared in two different manners: (1) time-dependent effect in the non-centrifugation portion, i.e., 2 vs. 48 h, as represented by the statistical symbol &#x201C;<sup>&#x2217;</sup>&#x201D; and (2) concentration-dependent effect in each time point, i.e., suspension vs. supernatant, as represented by the statistical symbol &#x201C;<sup>&#x2020;</sup>&#x201D;. We observed a significant decrease in fluorescence after 48 h at all concentrations of A&#x03B2;<sub>25-35</sub> (0.5&#x2013;10.0 &#x03BC;g/ml) when compared with 2 h incubation (<bold>Table <xref ref-type="table" rid="T2">2</xref></bold>), both in the non-centrifuged solution and in the supernatant of the centrifuged solution. These data suggest that incubating the peptide at RT for 48 h results in the formation of aggregates, as evidenced by the decreased FLCN absorbance in the supernatants of samples that were solubilized for 48 h as compared to those that were solubilized for 2 h prior to centrifugation. Based on our findings, non-centrifuged solutions were used for downstream experiments in order to ensure that astrocytes were exposed to aggregates of varying sizes. To address the question of whether oligomerization of A&#x03B2;<sub>25-35</sub> affects astrocyte proliferation, we treated non-serum-deprived primary astrocyte cultures for 12, 24, 36, or 48 h with graded concentrations of agA&#x03B2;<sub>25-35</sub> or non-agA&#x03B2;<sub>25-35</sub>. In contrast to our earlier findings using A&#x03B2;<sub>25-35</sub> (<bold>Figure <xref ref-type="fig" rid="F1">1A</xref></bold>), agA&#x03B2;<sub>25-35</sub> only significantly increased the rate of proliferation of non-serum-deprived astrocytes compared with control after 24 h of stimulation at a concentration of 3.0 &#x03BC;g/ml (<bold>Figure <xref ref-type="fig" rid="F4">4</xref></bold>).</p>
<table-wrap position="float" id="T2">
<label>Table 2</label>
<caption><p>Effect of time and fraction on A&#x03B2;<sub>25-35</sub> aggregation in solution<sup>&#x2021;</sup>.</p></caption>
<table cellspacing="5" cellpadding="5" frame="hsides" rules="groups">
<thead>
<tr>
<th valign="top" align="left">[A&#x03B2;<sub>25-35</sub>] (&#x03BC;g/ml)</th>
<th valign="top" align="center">Centrifugation</th>
<th valign="top" align="center">2 h, mean fluorescence intensity &#x00B1; SEM</th>
<th valign="top" align="center">48 h, mean fluorescence intensity &#x00B1; SEM</th>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left">0.5</td>
<td valign="top" align="center">-</td>
<td valign="top" align="center">3.20 &#x00B1; 1.21</td>
<td valign="top" align="center">1.20 &#x00B1; 0.18<sup>&#x2217;</sup></td>
</tr>
<tr>
<td valign="top" align="left"></td>
<td valign="top" align="center">+</td>
<td valign="top" align="center">2.00 &#x00B1; 0.77</td>
<td valign="top" align="center">0.9 &#x00B1; 0.08<sup>&#x2217;&#x2020;</sup></td>
</tr>
<tr>
<td valign="top" align="left">1.0</td>
<td valign="top" align="center">-</td>
<td valign="top" align="center">11.40 &#x00B1; 0.63</td>
<td valign="top" align="center">4.00 &#x00B1; 0.31<sup>&#x2217;&#x2217;&#x2217;&#x2217;</sup></td>
</tr>
<tr>
<td valign="top" align="left"></td>
<td valign="top" align="center">+</td>
<td valign="top" align="center">9.60 &#x00B1; 2.44</td>
<td valign="top" align="center">3.60 &#x00B1; 0.85<sup>&#x2217;&#x2217;&#x2217;&#x2020;&#x2020;&#x2020;</sup></td>
</tr>
<tr>
<td valign="top" align="left">3.0</td>
<td valign="top" align="center">-</td>
<td valign="top" align="center">34.20 &#x00B1; 1.76</td>
<td valign="top" align="center">22.70 &#x00B1; 0.76<sup>&#x2217;&#x2217;</sup></td>
</tr>
<tr>
<td valign="top" align="left"></td>
<td valign="top" align="center">+</td>
<td valign="top" align="center">21.5 &#x00B1; 4.00</td>
<td valign="top" align="center">9.00 &#x00B1; 0.76<sup>&#x2217;&#x2217;&#x2020;&#x2020;</sup></td>
</tr>
<tr>
<td valign="top" align="left">10.0</td>
<td valign="top" align="center">-</td>
<td valign="top" align="center">187.5 &#x00B1; 5.46</td>
<td valign="top" align="center">99.20 &#x00B1; 4.41<sup>&#x2217;&#x2217;&#x2217;&#x2217;</sup></td>
</tr>
<tr>
<td valign="top" align="left"></td>
<td valign="top" align="center">+</td>
<td valign="top" align="center">136.50 &#x00B1; 4.37</td>
<td valign="top" align="center">47.20 &#x00B1; 2.73<sup>&#x2217;&#x2217;&#x2217;&#x2217;&#x2020;&#x2020;&#x2020;&#x2020;</sup></td>
</tr>
<tr>
<td valign="top" align="left"></td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<attrib><italic><sup>&#x2021;</sup>Fluorescence intensity is measured in arbitrary units.; <sup>&#x2217;&#x2020;</sup><italic>p</italic> &#x003C; 0.025; <sup>&#x2217;&#x2217;&#x2020;&#x2020;</sup><italic>p</italic> &#x003C; 0.001; <sup>&#x2217;&#x2217;&#x2217;&#x2020;&#x2020;&#x2020;</sup><italic>p</italic> &#x003C; 0.005; <sup>&#x2217;&#x2217;&#x2217;&#x2217;&#x2020;&#x2020;&#x2020;&#x2020;</sup><italic>p</italic> &#x003C; 0.0005.</italic></attrib>
</table-wrap-foot>
</table-wrap>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption><p>The effect of A&#x03B2;<sub>25-35</sub> aggregation on the proliferation of non-serum-deprived primary astrocytes. Freshly prepared A&#x03B2;<sub>25-35</sub> was allowed to aggregate in PBS (pH 7.4) for 48 h; aggregation was confirmed by FLCN incorporation assay (<bold>Table <xref ref-type="table" rid="T2">2</xref></bold>). Non-serum-deprived astrocytes were treated with varying concentrations of agA&#x03B2;<sub>25-35</sub> (0.01&#x2013;3.0 &#x03BC;g/ml), and <sup>3</sup>H-thymidine incorporation assay was performed to measure rate of DNA synthesis. <sup>&#x2217;</sup><italic>p</italic> &#x003C; 0.05; <sup>&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.02; <sup>&#x2217;&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.001 (results were average values of three representative experiments).</p></caption>
<graphic xlink:href="fncel-11-00301-g004.tif"/>
</fig>
</sec>
<sec><title>Exposure to A&#x03B2;<sub>25-35</sub> During G<sub>1</sub> Phase Is Required to Stimulate Proliferation of Serum-Deprived Astrocytes</title>
<p>Finally, we examined whether the effect of A&#x03B2;<sub>25-35</sub> on astrocyte proliferation is phase-specific. A&#x03B2;<sub>25-35</sub> or CP (1.0 &#x03BC;g/ml) was added to serum-deprived astrocyte cultures at the time of serum up-shift or various times after serum up-shift (<italic>T</italic><sub>6</sub>, <italic>T</italic><sub>12</sub>, and <italic>T</italic><sub>16</sub>). All cultures were terminated at the peak of the S phase (<italic>T</italic><sub>24</sub>), and the rates of proliferation were determined using <sup>3</sup>H-thymidine incorporation. Consistent with our earlier results, we found that adding A&#x03B2;<sub>25-35</sub> at <italic>T</italic><sub>0</sub> significantly increased the rate of DNA synthesis at the peak of S phase (<italic>T</italic><sub>24</sub>) compared with control or CP (<italic>p</italic> &#x003C; 0.001; <bold>Figure <xref ref-type="fig" rid="F5">5A</xref></bold>). When A&#x03B2;<sub>25-35</sub> was added in the middle of G<sub>1</sub> phase at <italic>T</italic><sub>6</sub>, we observed a similar increase in the rate of DNA synthesis compared with CP or control (<italic>p</italic> &#x003C; 0.02). However, when addition was delayed until the G<sub>1</sub>/S phase transition point (<italic>T</italic><sub>12</sub>) or until the initiation of S phase, the rates of astrocyte proliferation were not significantly different among the A&#x03B2;<sub>25-35</sub>, CP, and control groups (<bold>Figure <xref ref-type="fig" rid="F5">5A</xref></bold>), suggesting that the effect of A&#x03B2;<sub>25-35</sub> on astrocyte proliferation is phase-specific, and initiated during the G<sub>1</sub> phase and before G<sub>1</sub>/S phase transition point.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption><p>Temporal effects of A&#x03B2;<sub>25-35</sub> on the proliferation of serum-deprived primary astrocytes. Newborn astrocytes were first serum-deprived and then re-entered into the cell cycle by serum up-shift. <bold>(A)</bold> Left, experimental approach; Right, A&#x03B2;<sub>25-35</sub> (1.0 &#x03BC;g/ml) or CP (1.0 &#x03BC;g/ml) was added to the cultures at varying times after serum up-shift (0, 6, 12, or 16 h). <bold>(B)</bold> Left, experimental approach; Right, A&#x03B2;<sub>25-35</sub> (1.0 &#x03BC;g/ml) was added to the cultures at different time points and then removed via medium changes after 3, 6, or 7 h of incubation. All cultures were terminated at <italic>T</italic><sub>24</sub>, and <sup>3</sup>H-thymidine incorporation assay was performed to measure rate of DNA synthesis. <sup>&#x2217;</sup><italic>p</italic> &#x003C; 0.05; <sup>&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.02; <sup>&#x2217;&#x2217;&#x2217;</sup><italic>p</italic> &#x003C; 0.001 (results were average values of three representative experiments).</p></caption>
<graphic xlink:href="fncel-11-00301-g005.tif"/>
</fig>
<p>We further defined the critical period of A&#x03B2;<sub>25-35</sub> exposure by using a &#x201C;delayed addition and early removal&#x201D; paradigm. In these experiments, we added A&#x03B2;<sub>25-35</sub> to the cultures at different points of the cell cycle and then changed the medium to remove A&#x03B2;<sub>25-35</sub> after varying exposure durations (3, 6, or 7 h); all cultures were terminated at the peak of the S phase (<italic>T</italic><sub>24</sub>), and the rate of proliferation was determined using <sup>3</sup>H-thymidine incorporation. We found that A&#x03B2;<sub>25-35</sub> significantly increased the rate of astrocyte proliferation as compared to control only if it was added to the culture during early to mid-G<sub>1</sub> phase (<italic>T</italic><sub>0</sub>, <italic>T</italic><sub>3</sub>, or <italic>T</italic><sub>6</sub>; <bold>Figure <xref ref-type="fig" rid="F5">5B</xref></bold>). When A&#x03B2;<sub>25-35</sub> was added to the cultures in late G<sub>1</sub> phase (<italic>T</italic><sub>9</sub>), there was no significant difference in the rate of DNA synthesis compared with control (<bold>Figure <xref ref-type="fig" rid="F5">5B</xref></bold>), regardless of whether the exposure duration was 3 (<italic>T</italic><sub>9</sub>&#x2013;<italic>T</italic><sub>12</sub>) or 7 h (<italic>T</italic><sub>9</sub>&#x2013;<italic>T</italic><sub>16</sub>). CP did not alter the rate of DNA synthesis during any of these exposure periods (data not shown). These results suggest that A&#x03B2;<sub>25-35</sub> affects the proliferation of astrocytes during early-to-mid-G<sub>1</sub> phase.</p>
</sec>
</sec>
<sec><title>Discussion</title>
<p>A definitive diagnosis of AD is based on histopathological evidence at autopsy or brain biopsy, including the presence of A&#x03B2; deposits, neuritic changes with formation of paired helical filaments and hyperphosphorylated tau, and reactive astrogliosis (<xref ref-type="bibr" rid="B63">Serrano-Pozo et al., 2011</xref>). Astrocytosis is widespread in the early phases of AD but declines as the disease progresses, indicating that gliosis may be an early pathogenic event (<xref ref-type="bibr" rid="B46">Pike et al., 1995a</xref>; <xref ref-type="bibr" rid="B57">Santillo et al., 2011</xref>; <xref ref-type="bibr" rid="B51">Rodriguez-Vieitez et al., 2015</xref>, <xref ref-type="bibr" rid="B52">2016</xref>; <xref ref-type="bibr" rid="B60">Scholl et al., 2015</xref>). <italic>In vitro</italic> studies consistently demonstrate that A&#x03B2; is neurotoxic and consequently induces neuritic changes (<xref ref-type="bibr" rid="B62">Sendrowski et al., 2015</xref>; <xref ref-type="bibr" rid="B54">Sadleir et al., 2016</xref>). Although pathological studies show that A&#x03B2;-containing senile plaques are often surrounded by reactive astrocytes, the relationship between different A&#x03B2; species and functional changes in astrocytes is less clear. Here, we hypothesize that A&#x03B2;<sub>25-35</sub> increases astrocyte proliferation, but that aggregation of A&#x03B2;<sub>25-35</sub> inhibits this effect.</p>
<p>Interestingly, although aberrant expression of mitotic regulators, such as cyclin c and binding partner Cdk8 have been observed in the astrocytes of AD brains (<xref ref-type="bibr" rid="B68">Ueberham et al., 2003</xref>), <italic>in vitro</italic> studies demonstrate highly variable and contrasting effects of A&#x03B2; on astrocytes (<xref ref-type="bibr" rid="B2">Agostinho et al., 2010</xref>), including induction of apoptosis (<xref ref-type="bibr" rid="B10">Brera et al., 2000</xref>; <xref ref-type="bibr" rid="B22">Hou et al., 2011</xref>; <xref ref-type="bibr" rid="B55">Saha and Biswas, 2015</xref>) and oxidative stress (<xref ref-type="bibr" rid="B10">Brera et al., 2000</xref>), as well as changes in morphology (<xref ref-type="bibr" rid="B56">Salinero et al., 1997</xref>) and proliferation (<xref ref-type="bibr" rid="B21">Hernandez-Guillamon et al., 2009</xref>). Our results show that A&#x03B2;<sub>25-35</sub> upregulates proliferation in both serum-deprived and non-serum-deprived astrocytes in time- and concentration-dependent manners as measured by <sup>3</sup>H-thymidine incorporation assay and BrdU staining (<bold>Figures <xref ref-type="fig" rid="F1">1</xref></bold>, <bold><xref ref-type="fig" rid="F2">2</xref></bold>); importantly, A&#x03B2;<sub>25-35</sub> did not induce cellular death in our experiments, as demonstrated by minimal cell death in trypan blue exclusion assay (&#x003C;2%). We found that CP (A&#x03B2;<sub>35-25</sub>) did not impact astrocyte proliferation, confirming the bio-specific effect of A&#x03B2;<sub>25-35</sub> on the rate of DNA synthesis in primary astrocytes depends on its amino acid sequence (<bold>Figures <xref ref-type="fig" rid="F1">1</xref></bold>, <bold><xref ref-type="fig" rid="F2">2</xref></bold>). Although increasing the concentration of A&#x03B2;<sub>25-35</sub> upregulated the rate of proliferation over a certain range (i.e., 0.01&#x2013;1.0 &#x03BC;g/ml), showing a clear concentration-effect of A&#x03B2;<sub>25-35</sub> on DNA synthesis in astroctyes, further increase of the A&#x03B2;<sub>25-35</sub> concentration to 3.0 &#x03BC;g/ml failed to enhance DNA synthesis (<bold>Figure <xref ref-type="fig" rid="F1">1</xref></bold>). While our data demonstrate a narrow concentration-effect window, this phenomenon has been reported in other biological systems, including that seen in astrocytes. For example, it was shown that just a 1% change in the concentration of isoflurane had a dramatic effect on astrocyte calcium signaling in ferret visual cortex (<xref ref-type="bibr" rid="B61">Schummers et al., 2008</xref>). Similarly, it has been shown that mitochondrial function is extremely sensitive to a narrow range of Ca<sup>2+</sup> ion concentrations (<xref ref-type="bibr" rid="B59">Schild et al., 2005</xref>), as is cellular survival in response to free zinc ions (<xref ref-type="bibr" rid="B9">Bozym et al., 2010</xref>). While the mechanisms underlying the concentration effects of each of these phenomena are currently unknown, one potential explanation of our data is that A&#x03B2;<sub>25-35</sub> follows a classical concentration-effect response via specific receptors; however, further research is required in order to elucidate the molecular basis of this response (<xref ref-type="bibr" rid="B56">Salinero et al., 1997</xref>; <xref ref-type="bibr" rid="B10">Brera et al., 2000</xref>; <xref ref-type="bibr" rid="B22">Hou et al., 2011</xref>; <xref ref-type="bibr" rid="B55">Saha and Biswas, 2015</xref>). Our data showing narrow effective concentration range on astrocyte proliferation do suggest a plausible explanation for astrocyte toxicity in advanced AD. In fact, others have shown that A&#x03B2;<sub>25-35</sub> is cytotoxic to astrocytes, those studies were carried out using concentrations 1000-fold higher than our current study; therefore, our results do not exclude the findings that high doses of A&#x03B2;<sub>25-35</sub> can be cytotoxic to astrocytes <italic>in vitro</italic>.</p>
<p>Our findings also demonstrate that the effect of A&#x03B2;<sub>25-35</sub> is cell cycle phase-specific. First, A&#x03B2;<sub>25-35</sub> increases the rate of DNA synthesis in serum-deprived astrocytes during the S phase but not during G<sub>1</sub> phase (<bold>Figure <xref ref-type="fig" rid="F2">2</xref></bold>). Second, the timing of exposure to A&#x03B2;<sub>25-35</sub> was critical. To upregulate astrocyte proliferation, A&#x03B2;<sub>25-35</sub> needed to be added to astrocytes during early-to-mid-G<sub>1</sub> phase. If A&#x03B2;<sub>25-35</sub> was added any later than 6 h into G<sub>1</sub>, the rate of proliferation was not impacted (<bold>Figure <xref ref-type="fig" rid="F5">5</xref></bold>). These findings offer novel insights into the effect of A&#x03B2;<sub>25-35</sub> on astrocyte proliferation, and the mechanisms underlying the phase specificity are currently under investigation in our laboratory.</p>
<p>We showed that aggregation of A&#x03B2;<sub>25-35</sub> impaired its upregulatory effect on astrocyte proliferation, as agA&#x03B2;<sub>25-35</sub> increased DNA synthesis relative to control only at a concentration of 3.0 &#x03BC;g/ml and only at <italic>T</italic><sub>24</sub> (i.e., 12 h into the S phase, <bold>Figure <xref ref-type="fig" rid="F4">4</xref></bold>). Senile plaques, a hallmark feature of AD pathology, are made up of fibrillar or &#x03B2;-sheet aggregates of amyloid peptide; amyloid deposition has been shown to occur progressively over the course of the disease and has been proposed as a biomarker for disease staging (<xref ref-type="bibr" rid="B26">Jack et al., 2013</xref>). However, our results clearly show that aggregation of amyloid peptide limits its ability to stimulate astrocytes. As astrocyte activation precedes plaque formation in AD patients (<xref ref-type="bibr" rid="B51">Rodriguez-Vieitez et al., 2015</xref>), it is conceivable that initial A&#x03B2; deposition increases astrocyte proliferation and leads to reactive astrocytosis during the early stages of amyloid deposition, but that as senile plaques by amyloid aggregation are formed, the rate of astrocyte reactivation slows down.</p>
</sec>
<sec><title>Conclusion</title>
<p>Our study is the first to show evidence of the upregulatory effect of A&#x03B2;<sub>25-35</sub> on DNA synthesis during the S phase of the primary astrocyte cell cycle. Our results demonstrate that A&#x03B2;<sub>25-35</sub> affected the cell cycle only when astrocytes were exposed during early-to-mid-G<sub>1</sub> phase. Exposing primary astrocytes to A&#x03B2;<sub>25-35</sub> 3 h prior to G<sub>1</sub>/S intersection (<italic>T</italic><sub>9</sub>) failed to increase DNA synthesis in the S phase, irrespective of exposure duration. Therefore, these results suggest the temporal importance of A&#x03B2; exposure preceding the late G<sub>1</sub> phase restriction point of the astrocyte cell cycle. The time-based specificity of the effect of A&#x03B2;<sub>25-35</sub> on the astrocyte cell cycle thus points to the possibility that this peptide participates in the complex array of biochemical and molecular events that confer commitment to cell-cycle progression; further investigation is required to determine the exact mechanisms responsible. Additionally, while the present study focuses on the effect of A&#x03B2;<sub>25-35</sub> on astrocytes, it would also be worthwhile to examine its impact on the cellular functions and rate of proliferation of other cells important for brain function, such as microglia, which have crucial roles in central nervous system immunity, and endothelial cells, which maintain the blood&#x2013;brain barrier.</p>
</sec>
<sec><title>Author Contributions</title>
<p>Experiments were conceived and designed by EO, TL, and RC. Experiments were performed by EO and RC. Data were analyzed by EO, KR, and RC. Reagents/materials/tools provided by TL. Manuscript was written and prepared by EO, KR, and RC. All authors reviewed and approved the final version of the manuscript.</p>
</sec>
<sec><title>Conflict of Interest Statement</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
</body>
<back>
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