Survey of helium weak stars

The spectra of a dozen stars were obtained in which the colors are bluer than expected according to their spectral types. Eight of them are helium weak. With these objects the percentage of stars of this type is increased by 50 %. The paper in full will be published elsewhere.

Guardado en:
Detalles Bibliográficos
Autores principales: Jaschek, Carlos, Jaschek, Mercedes, Arnal, Edmundo Marcelo
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1970
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/97666
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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