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dc.date.accessioned 2022-09-13T14:41:02Z
dc.date.available 2022-09-13T14:41:02Z
dc.date.issued 1988
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/142003
dc.description.abstract The new version of the Wilson and Devinney synthetic method is employed to study the BV photometry and the radial velocity curves for both components of V508 Ophiuchi. The results show that this binary is a normal A-type W UMa star with a mass ratio of 0.53 and with a relatively low degree of over–contact (about 10%). The study is completed with the determination of absolute values for the dimensions, masses, and luminosities of the system. The unusual behaviour of previous light curves obtained by other authors might roughly be explained by means of selective emission located in the contact zone. en
dc.language es es
dc.subject Galaxia es
dc.subject v508 oph es
dc.title Simultaneous analysis of light and radial velocity curves of V508 Ophiuchi en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Lapasset, E. es
sedici.creator.person Gómez, M. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 34 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)