Órbita de ε Coronae Austrinae

The W UMa system of ε Coronae Austrinae only shows the spectrum of one of the components which corresponds to type FOV. Since the amplitudes of the two light minima are approximately equal, the two components must have comparable surface brightness and, as a consequence, the fact that only one spect...

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Guardado en:
Detalles Bibliográficos
Autores principales: Hernández, Carlos A., Sahade, Jorge
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1969
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/94437
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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