Mass Loss from Massive Zero-Metallicity Stars

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Authors	KRTIČKA Jiří KUBÁT Jiří
Year of publication	2006
Type	Article in Proceedings
Conference	Stellar Evolution at Low Metallicity: Mass Loss, Explosions
MU Faculty or unit	Faculty of Science
Citation
Web	http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ASPC..353..133K&db_key=AST&data_type=HTML&format=&high=403a2464f518671
Field	Astronomy and astrophysics
Keywords	stars: mass-loss - stars: winds outflows -- stars: early-type - stars: circumstellar matter
Description	We show that the radiative force is not able to drive a stellar wind from non-rotating hot massive zero-metallicity stars. This means that stellar winds from stationary massive hot first generation stars are unlikely. We study the possibility of expulsion of chemically homogeneous winds and the role of minor isotopes.
Related projects:	Hydrodynamics of stellar wind of hot stars Circumstellar envelopes of hot stars