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dc.date.accessioned 2022-02-15T13:44:48Z
dc.date.available 2022-02-15T13:44:48Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/131094
dc.description.abstract A detailed analysis by means of the Wilson and Devinney method of the UBV photometry of BR Muscae is shown. Different values are investigated of the mass-ratio q between 0.4 and 1.5. Finally, it is established that the best solutions correspond to values of q close to unity. A degree of contact of about 11% is found. According to the period-spectral type relation, BR Muscae appears to be little evolved. Its relation with the remaining massive contact binaries is shortly discussed. es
dc.language es es
dc.subject Galaxias es
dc.subject br mus es
dc.title BR Muscae: un sistema temprano de componentes similares en contacto marginal es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Gómez, M.N. es
sedici.creator.person Lapasset, E. 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. 32 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) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)