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HOT STAR WINDS AND INTERFEROMETRY: ACHERNAR AND n CARINAE

The considerable radiative pressure of massive hot stars is a very eficient engine for the ejection of stellar winds. In addition, hot stars are often also fast rotators. In this case, their attened photosphere results in overheated polar caps through the Von Zeipel efect, and a low e ective gravit...

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Publicado en:Revista Mexicana de Astronomía y Astrofísica
Principais autores: P. Kervella, A. Mérand
Formato: Artigo
Idioma:Inglês
Publicado: Universidad Nacional Autónoma de México 2010
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Acceso en liña:https://www.redalyc.org/articulo.oa?id=57115706014
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