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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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2010
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57115706014 |
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