High and intermediate-resolution spectroscopy of Be stars : An atlas of Hγ, He I 4471 and Mg II 4481 lines
The definition of Be stars (Jaschek et al. 1981) as non-supergiant B stars which at least once have shown some emission in the Balmer lines implies a vast phenomenology whose characteristics, the evolution of their understanding and the questions which still remain open have been widely reviewed in...
Guardado en:
| Autores principales: | Chauville, J., Zorec, Juan, Ballereau, Dominique, Morrell, Nidia Irene, Cidale, Lydia Sonia, García, A. |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2001
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/2084 http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2001A%2526A...378..861CFUL |
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