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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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Bibliographic Details
Published in:Revista Mexicana de Astronomía y Astrofísica
Main Authors: Aaron Flores, Gloria Koenigsberger, Octavio Cardona, Lelio de la Cruz
Format: Artigo
Language:Inglês
Published: Universidad Nacional Autónoma de México 2011
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Online Access:https://www.redalyc.org/articulo.oa?id=57120957006
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