U, B, V light curves of CO Lacertae

U, B, V light curves of CO Lacertae

CO Lacertae is one of the very few known binaries with both a short period of apsidal motion and good M, L, R data. The new U, B, V light curves presented here provide two times of minima and a check on Semeniuk's value for P(aps). This is the first published example of an eclipsing binary anal...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astrophysics and space science 1983-01, Vol.89 (1 Ja), p.5-14
Hauptverfasser: Wilson, R. E., Woodward, E. J.
Format: Artikel
Sprache:eng
Schlagworte:
Astrophysics
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 14
container_issue 1 Ja
container_start_page 5
container_title Astrophysics and space science
container_volume 89
creator Wilson, R. E.
Woodward, E. J.
description CO Lacertae is one of the very few known binaries with both a short period of apsidal motion and good M, L, R data. The new U, B, V light curves presented here provide two times of minima and a check on Semeniuk's value for P(aps). This is the first published example of an eclipsing binary analyzed in terms of a physical model (as opposed to a model based on spherical or ellipsoidal star figures) which allows for eccentric orbit effects. The light curves show some peculiarities - particularly a large, probably intrinsic, scatter.
doi_str_mv 10.1007/BF01008381
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_23118152</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>23118152</sourcerecordid><originalsourceid>FETCH-LOGICAL-c281t-5bce801e4112616273fcfd2d513f6b4bb7ca4ca0619fe3eb4828af0864da94433</originalsourceid><addsrcrecordid>eNpFkMFLwzAcRoMoWKcXzx4CggdZNb8kTZOjK06Fwi5OdgtpmmilW2fSCvvvrVTw9Pjg8R0eQpdA7oCQ_H6xJCMlk3CEEshymiouNscoIYTwVHCyOUVnMX6OUwmVJ-h6PceLOX7DbfP-0WM7hG8XcedxscKlsS70xp2jE2_a6C7-OEPr5eNr8ZyWq6eX4qFMLZXQp1llnSTgOAAVIGjOvPU1rTNgXlS8qnJruDVEgPKOuYpLKo0nUvDaKM4Zm6Gb6Xcfuq_BxV5vm2hd25qd64aoKQOQkNFRvJ1EG7oYg_N6H5qtCQcNRP920P8dRvlqkncmGr3rQ9SgJBt75JIx9gMhwVSc</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>23118152</pqid></control><display><type>article</type><title>U, B, V light curves of CO Lacertae</title><source>Springer Nature - Complete Springer Journals</source><source>NASA Technical Reports Server</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><creator>Wilson, R. E. ; Woodward, E. J.</creator><creatorcontrib>Wilson, R. E. ; Woodward, E. J.</creatorcontrib><description>CO Lacertae is one of the very few known binaries with both a short period of apsidal motion and good M, L, R data. The new U, B, V light curves presented here provide two times of minima and a check on Semeniuk's value for P(aps). This is the first published example of an eclipsing binary analyzed in terms of a physical model (as opposed to a model based on spherical or ellipsoidal star figures) which allows for eccentric orbit effects. The light curves show some peculiarities - particularly a large, probably intrinsic, scatter.</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1007/BF01008381</identifier><language>eng</language><publisher>Legacy CDMS</publisher><subject>Astrophysics</subject><ispartof>Astrophysics and space science, 1983-01, Vol.89 (1 Ja), p.5-14</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c281t-5bce801e4112616273fcfd2d513f6b4bb7ca4ca0619fe3eb4828af0864da94433</citedby><cites>FETCH-LOGICAL-c281t-5bce801e4112616273fcfd2d513f6b4bb7ca4ca0619fe3eb4828af0864da94433</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,4010,27900,27901,27902</link.rule.ids></links><search><creatorcontrib>Wilson, R. E.</creatorcontrib><creatorcontrib>Woodward, E. J.</creatorcontrib><title>U, B, V light curves of CO Lacertae</title><title>Astrophysics and space science</title><description>CO Lacertae is one of the very few known binaries with both a short period of apsidal motion and good M, L, R data. The new U, B, V light curves presented here provide two times of minima and a check on Semeniuk's value for P(aps). This is the first published example of an eclipsing binary analyzed in terms of a physical model (as opposed to a model based on spherical or ellipsoidal star figures) which allows for eccentric orbit effects. The light curves show some peculiarities - particularly a large, probably intrinsic, scatter.</description><subject>Astrophysics</subject><issn>0004-640X</issn><issn>1572-946X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1983</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNpFkMFLwzAcRoMoWKcXzx4CggdZNb8kTZOjK06Fwi5OdgtpmmilW2fSCvvvrVTw9Pjg8R0eQpdA7oCQ_H6xJCMlk3CEEshymiouNscoIYTwVHCyOUVnMX6OUwmVJ-h6PceLOX7DbfP-0WM7hG8XcedxscKlsS70xp2jE2_a6C7-OEPr5eNr8ZyWq6eX4qFMLZXQp1llnSTgOAAVIGjOvPU1rTNgXlS8qnJruDVEgPKOuYpLKo0nUvDaKM4Zm6Gb6Xcfuq_BxV5vm2hd25qd64aoKQOQkNFRvJ1EG7oYg_N6H5qtCQcNRP920P8dRvlqkncmGr3rQ9SgJBt75JIx9gMhwVSc</recordid><startdate>19830101</startdate><enddate>19830101</enddate><creator>Wilson, R. E.</creator><creator>Woodward, E. J.</creator><scope>CYE</scope><scope>CYI</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19830101</creationdate><title>U, B, V light curves of CO Lacertae</title><author>Wilson, R. E. ; Woodward, E. J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c281t-5bce801e4112616273fcfd2d513f6b4bb7ca4ca0619fe3eb4828af0864da94433</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1983</creationdate><topic>Astrophysics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wilson, R. E.</creatorcontrib><creatorcontrib>Woodward, E. J.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wilson, R. E.</au><au>Woodward, E. J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>U, B, V light curves of CO Lacertae</atitle><jtitle>Astrophysics and space science</jtitle><date>1983-01-01</date><risdate>1983</risdate><volume>89</volume><issue>1 Ja</issue><spage>5</spage><epage>14</epage><pages>5-14</pages><issn>0004-640X</issn><eissn>1572-946X</eissn><abstract>CO Lacertae is one of the very few known binaries with both a short period of apsidal motion and good M, L, R data. The new U, B, V light curves presented here provide two times of minima and a check on Semeniuk's value for P(aps). This is the first published example of an eclipsing binary analyzed in terms of a physical model (as opposed to a model based on spherical or ellipsoidal star figures) which allows for eccentric orbit effects. The light curves show some peculiarities - particularly a large, probably intrinsic, scatter.</abstract><cop>Legacy CDMS</cop><doi>10.1007/BF01008381</doi><tpages>10</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0004-640X
ispartof Astrophysics and space science, 1983-01, Vol.89 (1 Ja), p.5-14
issn 0004-640X
1572-946X
language eng
recordid cdi_proquest_miscellaneous_23118152
source Springer Nature - Complete Springer Journals; NASA Technical Reports Server; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals
subjects Astrophysics
title U, B, V light curves of CO Lacertae
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-01T14%3A35%3A33IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=U,%20B,%20V%20light%20curves%20of%20CO%20Lacertae&rft.jtitle=Astrophysics%20and%20space%20science&rft.au=Wilson,%20R.%20E.&rft.date=1983-01-01&rft.volume=89&rft.issue=1%20Ja&rft.spage=5&rft.epage=14&rft.pages=5-14&rft.issn=0004-640X&rft.eissn=1572-946X&rft_id=info:doi/10.1007/BF01008381&rft_dat=%3Cproquest_cross%3E23118152%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=23118152&rft_id=info:pmid/&rfr_iscdi=true