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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Kaydedildi:
Detaylı Bibliyografya
Yayımlandı:Revista Mexicana de Astronomía y Astrofísica
Asıl Yazarlar: Aaron Flores, Gloria Koenigsberger, Octavio Cardona, Lelio de la Cruz
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: Universidad Nacional Autónoma de México 2011
Konular:
Física, Astronomía y Matemáticas
Rayet
outflows
stars: Wolf
stars: winds
Stars: individual (EZ CMa = HD 50896)
Online Erişim:https://www.redalyc.org/articulo.oa?id=57120957006
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