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dc.provenanceCONICET-
dc.creatorLiu, L.-
dc.creatorQian, S. B.-
dc.creatorFernandez Lajus, Eduardo Eusebio-
dc.date2017-05-12T19:42:21Z-
dc.date2017-05-12T19:42:21Z-
dc.date2011-07-
dc.date2017-03-27T15:54:41Z-
dc.date.accessioned2019-04-29T15:33:55Z-
dc.date.available2019-04-29T15:33:55Z-
dc.date.issued2011-07-
dc.identifierLiu, L.; Qian, S. B.; Fernandez Lajus, Eduardo Eusebio; Two extreme contact binary systems in the nearest globular cluster M4; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 415; 2; 7-2011; 1509-1522-
dc.identifier0035-8711-
dc.identifierhttp://hdl.handle.net/11336/16410-
dc.identifier1365-2966-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/296662-
dc.descriptionWe present the results of photometric solutions for two contact binaries in the nearby globular cluster M4. We estimate their physical parameters using the light-curve program of the Wilson Devinney code. These systems have quite different mass ratios, which indicates that they did not form at the same time. V47 is an extreme mass-ratio system (q =0.123 ±0.002) being dissimilar to the same kind of field contact binaries. V53 is a high mass-ratio (q =1.230 ±0.004), deep-contact (f =79.7 ±1.9 per cent) system. It is also a blue straggler.-
dc.descriptionFil: Liu, L.. Chinese Academy Of Sciences; República de China-
dc.descriptionFil: Qian, S. B.. Chinese Academy Of Sciences; República de China-
dc.descriptionFil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina; Argentina-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherOxford University Press-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1111/j.1365-2966.2011.18791.x-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2011.18791.x-
dc.rightsinfo:eu-repo/semantics/restrictedAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.source.urihttp://hdl.handle.net/11336/16410-
dc.subjectEclipsing binaries-
dc.subjectV53 (estrella)-
dc.subjectV47 (estrella)-
dc.subjectEvolution of stars-
dc.subjectBlue stragglers-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleTwo extreme contact binary systems in the nearest globular cluster M4-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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