Photometric and spectroscopic variations of the Be star HD 112999

Be objects are stars of B spectral type showing lines of the Balmer series in emission. The presence of these lines is attributed to the existence of an extended envelope, disk type, around them. Some stars are observed in both the Be and normal B-type spectroscopic states and they are known as tran...

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Detalles Bibliográficos
Autores principales:	Weidmann, Walter Alfredo, Gamen, Roberto Claudio, Aidelman, Yael Judith, Ferrero Sosa, Gabriel Antonio, Corti, Mariela Alejandra
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2013
Materias:	Astronomía Física Ciencias Naturales Ciencias Exactas Stars: emission-line Stars: be Stars: individual: hd 112999 Stars: variables: general
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/93600 https://arxiv.org/abs/1305.7098
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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