dc.creator | Ostrov, Pablo Gabriel | |
dc.creator | Lapasset, Emilio | |
dc.date | 2003 | |
dc.date | 2019-11-04T16:43:07Z | |
dc.identifier | http://sedici.unlp.edu.ar/handle/10915/84850 | |
dc.identifier | issn:0035-8711 | |
dc.description | We 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.description | Facultad de Ciencias Astronómicas y Geofísicas | |
dc.format | application/pdf | |
dc.format | 141-146 | |
dc.language | en | |
dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
dc.subject | Ciencias Astronómicas | |
dc.subject | Binaries: Eclipsing | |
dc.subject | Stars: Early type | |
dc.subject | Stars: Fundamental parameters | |
dc.subject | Stars: Individual: Sk 67°105 | |
dc.title | The O4f + O6V eclipsing binary system Sk‒67°105 in the Large Magellanic Cloud | |
dc.type | Articulo | |
dc.type | Articulo | |