The O4f + O6V eclipsing binary system Sk‒67°105 in the Large Magellanic Cloud

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...

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Detalles Bibliográficos
Autores principales: Ostrov, Pablo Gabriel, Lapasset, Emilio
Formato: Articulo
Lenguaje:Inglés
Publicado: 2003
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84850
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