B stars in open clusters: fundamental parameters

We use the BCD spectrophotometric classification system to derive fundamental parameters of B stars in NGC 2439, NGC 3766 and NGC 6087. We are able to perform a complete study of each open cluster by deriving spectral classification of its members, distance modulus and age as well.

Guardado en:
Detalles Bibliográficos
Autores principales: Aidelman, Yael Judith, Cidale, Lydia Sonia, Zorec, Juan, Arias, María Laura
Formato: Articulo Comunicacion
Lenguaje:Inglés
Publicado: 2011
Materias:
Ciencias Astronómicas
Ciencias Exactas
Be
Stars: distances
Stars: emission-line
Stars: fundamental parameters
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84058
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
Descripción
Sumario:We use the BCD spectrophotometric classification system to derive fundamental parameters of B stars in NGC 2439, NGC 3766 and NGC 6087. We are able to perform a complete study of each open cluster by deriving spectral classification of its members, distance modulus and age as well.

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