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dc.date.accessioned 2022-08-30T12:47:08Z
dc.date.available 2022-08-30T12:47:08Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/141219
dc.description.abstract The UBV light curves of the early-type contact binary V393 Cen are analysed by means of the computational method of Wilson and Devinney. Different solutions, corresponding to values of the mass-ratio between 0.60 and 1.90, are presented. All them fit the observed data correctly. The remaining photometric parameters and, particularly, the percentage of overcontact, the difference of temperature between the components and the orbital inclination, are well defined. The cause of the photometric indetermination of the system mass-ratio is shortly discussed. en
dc.language es es
dc.subject Galaxia es
dc.subject v393 cen es
dc.title Photometric analysis of the early-type contact binary V393 Centauri en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Lapasset, E. es
sedici.creator.person Gómez, M. es
sedici.creator.person Clariá, J.J. 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. 33 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)