dc.creatorOstrov, Pablo Gabriel
dc.creatorLapasset, Emilio
dc.date2003
dc.date2019-11-04T16:43:07Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/84850
dc.identifierissn:0035-8711
dc.descriptionWe present a new V light curve of the early type Magellanic eclipsing binary Sk-67°105, based on charge-coupled device images obtained at CASLEO. We perform an analysis of our data, together with published radial velocities, deriving the following masses and radii: M<SUB>1</SUB> = 48.3 M⊙, R<SUB>1</SUB> = 16.9 R⊙ for the O4f component and M<SUB>2</SUB> = 31.4 M⊙, R<SUB>2</SUB> = 13.8 R⊙ for the O6 component. We found that this system is the brightest member of a tight star cluster, belonging to an OB association.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format141-146
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectBinaries: Eclipsing
dc.subjectStars: Early type
dc.subjectStars: Fundamental parameters
dc.subjectStars: Individual: Sk 67°105
dc.titleThe O4f + O6V eclipsing binary system Sk‒67°105 in the Large Magellanic Cloud
dc.typeArticulo
dc.typeArticulo


Este ítem pertenece a la siguiente institución