The spectroscopic orbits and physical parameters of GG Carinae

Aims. GG Car is an eclipsing binary classified as a B[e] supergiant star. The aims of our study are to improve the orbital elements of the binary system in order to obtain the actual orbital period of this system. We also compare the spectral energy distribution of the observed fluxes over a wide wa...

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Detalles Bibliográficos
Autores principales:	Marchiano, Paula Esther, Brandi, Estela, Muratore, María Florencia, Quiroga, Claudio Martín, Ferrer, Osvaldo Eduardo, García, Lía Guillermina
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2012
Materias:	Ciencias Astronómicas binaries: eclipsing stars: emission-line, Be stars: individual: GG Car techniques: spectroscopic
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84274
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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