Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods
Small-amplitude red variables (SARVs) are M giants or supergiants which are pulsating with small amplitudes (up to 2.5 mag) and with time scales of 20-200 days or more. This paper reports on a 10-yr study of about two dozen SARVs, carried out through the American Association of Variable Star Observe...
Gespeichert in:
Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1996-02, Vol.108 (720), p.139-145 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 145 |
---|---|
container_issue | 720 |
container_start_page | 139 |
container_title | Publications of the Astronomical Society of the Pacific |
container_volume | 108 |
creator | Percy, John R. Desjardins, Adrien Yu, Lawrence Landis, Howard J. |
description | Small-amplitude red variables (SARVs) are M giants or supergiants which are pulsating with small amplitudes (up to 2.5 mag) and with time scales of 20-200 days or more. This paper reports on a 10-yr study of about two dozen SARVs, carried out through the American Association of Variable Star Observers (AAVSO) photoelectric photometry program. It has provided detailed information on the regularity, period, and amplitude of these stars. Most have well-defined periods in the 20-200 day range.Several also have a long secondary period. One (W Boo) appears to have two periods with a ratio of 2.3. |
doi_str_mv | 10.1086/133703 |
format | Article |
fullrecord | <record><control><sourceid>jstor_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1086_133703</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>40680697</jstor_id><sourcerecordid>40680697</sourcerecordid><originalsourceid>FETCH-LOGICAL-c275t-173ab6bf762a5c8076c710cb03638368dbbd103bb277495f097be9eed19b03233</originalsourceid><addsrcrecordid>eNo90EtLAzEUBeAgCtaq_0DIyt3ozdxOknE3FF8w0GK1CzdDXtOmzHRKkgr-eysVV2fznbM4hFwzuGMg-T1DFIAnZMQKlBlKgadkBACTjOcSzslFjBsAxiSDEflc9KrrsqrfdT7traNvztKlCl7pzkXqtzStHa2q5WJG5-shDa5zJgVv6DwMq6D6B1r71TrR6T58HQpqa-ncBT_YeEnOWtVFd_WXY_Lx9Pg-fcnq2fPrtKozk4siZUyg0ly3gueqMBIEN4KB0YAcJXJptbYMUOtciElZtFAK7UrnLCsPJkcck9vjrglDjMG1zS74XoXvhkHz-0hzfOQAb45wE9MQ_tUEuAReCvwBkRxbBA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods</title><source>Jstor Complete Legacy</source><source>Institute of Physics Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Percy, John R. ; Desjardins, Adrien ; Yu, Lawrence ; Landis, Howard J.</creator><creatorcontrib>Percy, John R. ; Desjardins, Adrien ; Yu, Lawrence ; Landis, Howard J.</creatorcontrib><description>Small-amplitude red variables (SARVs) are M giants or supergiants which are pulsating with small amplitudes (up to 2.5 mag) and with time scales of 20-200 days or more. This paper reports on a 10-yr study of about two dozen SARVs, carried out through the American Association of Variable Star Observers (AAVSO) photoelectric photometry program. It has provided detailed information on the regularity, period, and amplitude of these stars. Most have well-defined periods in the 20-200 day range.Several also have a long secondary period. One (W Boo) appears to have two periods with a ratio of 2.3.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/133703</identifier><language>eng</language><publisher>American Institute of Physics</publisher><subject>Astronomical magnitude ; Astronomical photometry ; Autocorrelation ; Light curves ; Mathematical minima ; Stars ; Supergiant stars ; Variable stars ; Visible spectrum ; Weak minimum</subject><ispartof>Publications of the Astronomical Society of the Pacific, 1996-02, Vol.108 (720), p.139-145</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c275t-173ab6bf762a5c8076c710cb03638368dbbd103bb277495f097be9eed19b03233</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/40680697$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/40680697$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,776,780,799,27901,27902,57992,58225</link.rule.ids></links><search><creatorcontrib>Percy, John R.</creatorcontrib><creatorcontrib>Desjardins, Adrien</creatorcontrib><creatorcontrib>Yu, Lawrence</creatorcontrib><creatorcontrib>Landis, Howard J.</creatorcontrib><title>Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods</title><title>Publications of the Astronomical Society of the Pacific</title><description>Small-amplitude red variables (SARVs) are M giants or supergiants which are pulsating with small amplitudes (up to 2.5 mag) and with time scales of 20-200 days or more. This paper reports on a 10-yr study of about two dozen SARVs, carried out through the American Association of Variable Star Observers (AAVSO) photoelectric photometry program. It has provided detailed information on the regularity, period, and amplitude of these stars. Most have well-defined periods in the 20-200 day range.Several also have a long secondary period. One (W Boo) appears to have two periods with a ratio of 2.3.</description><subject>Astronomical magnitude</subject><subject>Astronomical photometry</subject><subject>Autocorrelation</subject><subject>Light curves</subject><subject>Mathematical minima</subject><subject>Stars</subject><subject>Supergiant stars</subject><subject>Variable stars</subject><subject>Visible spectrum</subject><subject>Weak minimum</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1996</creationdate><recordtype>article</recordtype><recordid>eNo90EtLAzEUBeAgCtaq_0DIyt3ozdxOknE3FF8w0GK1CzdDXtOmzHRKkgr-eysVV2fznbM4hFwzuGMg-T1DFIAnZMQKlBlKgadkBACTjOcSzslFjBsAxiSDEflc9KrrsqrfdT7traNvztKlCl7pzkXqtzStHa2q5WJG5-shDa5zJgVv6DwMq6D6B1r71TrR6T58HQpqa-ncBT_YeEnOWtVFd_WXY_Lx9Pg-fcnq2fPrtKozk4siZUyg0ly3gueqMBIEN4KB0YAcJXJptbYMUOtciElZtFAK7UrnLCsPJkcck9vjrglDjMG1zS74XoXvhkHz-0hzfOQAb45wE9MQ_tUEuAReCvwBkRxbBA</recordid><startdate>19960201</startdate><enddate>19960201</enddate><creator>Percy, John R.</creator><creator>Desjardins, Adrien</creator><creator>Yu, Lawrence</creator><creator>Landis, Howard J.</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19960201</creationdate><title>Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods</title><author>Percy, John R. ; Desjardins, Adrien ; Yu, Lawrence ; Landis, Howard J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c275t-173ab6bf762a5c8076c710cb03638368dbbd103bb277495f097be9eed19b03233</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1996</creationdate><topic>Astronomical magnitude</topic><topic>Astronomical photometry</topic><topic>Autocorrelation</topic><topic>Light curves</topic><topic>Mathematical minima</topic><topic>Stars</topic><topic>Supergiant stars</topic><topic>Variable stars</topic><topic>Visible spectrum</topic><topic>Weak minimum</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Percy, John R.</creatorcontrib><creatorcontrib>Desjardins, Adrien</creatorcontrib><creatorcontrib>Yu, Lawrence</creatorcontrib><creatorcontrib>Landis, Howard J.</creatorcontrib><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Percy, John R.</au><au>Desjardins, Adrien</au><au>Yu, Lawrence</au><au>Landis, Howard J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1996-02-01</date><risdate>1996</risdate><volume>108</volume><issue>720</issue><spage>139</spage><epage>145</epage><pages>139-145</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>Small-amplitude red variables (SARVs) are M giants or supergiants which are pulsating with small amplitudes (up to 2.5 mag) and with time scales of 20-200 days or more. This paper reports on a 10-yr study of about two dozen SARVs, carried out through the American Association of Variable Star Observers (AAVSO) photoelectric photometry program. It has provided detailed information on the regularity, period, and amplitude of these stars. Most have well-defined periods in the 20-200 day range.Several also have a long secondary period. One (W Boo) appears to have two periods with a ratio of 2.3.</abstract><pub>American Institute of Physics</pub><doi>10.1086/133703</doi><tpages>7</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6280 |
ispartof | Publications of the Astronomical Society of the Pacific, 1996-02, Vol.108 (720), p.139-145 |
issn | 0004-6280 1538-3873 |
language | eng |
recordid | cdi_crossref_primary_10_1086_133703 |
source | Jstor Complete Legacy; Institute of Physics Journals; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
subjects | Astronomical magnitude Astronomical photometry Autocorrelation Light curves Mathematical minima Stars Supergiant stars Variable stars Visible spectrum Weak minimum |
title | Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-04T22%3A19%3A11IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Small-Amplitude%20Red%20Variables%20in%20the%20AAVSO%20Photoelectric%20Program:%20Light%20Curves%20and%20Periods&rft.jtitle=Publications%20of%20the%20Astronomical%20Society%20of%20the%20Pacific&rft.au=Percy,%20John%20R.&rft.date=1996-02-01&rft.volume=108&rft.issue=720&rft.spage=139&rft.epage=145&rft.pages=139-145&rft.issn=0004-6280&rft.eissn=1538-3873&rft_id=info:doi/10.1086/133703&rft_dat=%3Cjstor_cross%3E40680697%3C/jstor_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_jstor_id=40680697&rfr_iscdi=true |