WIND STRUCTURE OF THE WOLF-RAYET STAR EZ CMA=HD 50896
The Wolf-Rayet star HD 50896 (EZ CMa=WR6) is well-known for the emission-line profile variability that occurs on a 3.7-day timescale. In particular, the shape of the N V 4604-21 doublet changes from a P Cygni profile to one in which no blue-shifted absorption component is present. In this paper we u...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2011
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57120957006 |
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