Properties of massive stars in Galactic binary systems

En el marco del proyecto OWN, usamos datos espectroscópicos de alta resolución de la binaria masiva HD 54662 para medir velocidades radiales y desentramar los espectros de las dos componentes del sistema, que hemos clasificado como 06.5 Vz(n) y 07.5 Vz. Obtenemos una nueva solución orbital espectros...

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Detalles Bibliográficos
Autores principales:	Sabín-Sanjulián, C., Barbá, Rodolfo Héctor, Gamen, Roberto Claudio, Arias, J. A.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2019
Materias:	Ciencias Astronómicas stars: massive stars: binaries stars: atmospheres stars: fundamental parameters
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/169630
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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