Confirmation and revision on the orbital period change of the possible type Ia supernova progenitor V617 Sagittarii

This work reports new photometric results of eclipsing cataclysmic variable V617 Sagittarii (V617 Sgr). We analyzed the orbital period change of V617 Sgr by employing three new (since 2010) CCD eclipse timings along with all the available data from the literature. It was found that the orbital perio...

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Detalles Bibliográficos
Autores principales:	Shi, Guang, Qian, Sheng Bang, Fernández Lajús, Eduardo
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2014
Materias:	Ciencias Astronómicas binaries: close binaries: eclipsing stars: evolution stars: individual (V617 Sgr) stars: winds, outflows
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85208
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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