Mass Loss from Massive Zero-Metallicity Stars

Details Mass Loss from Massive Zero-Metallicity Stars Mass Loss from Massive Zero-Metallicity Stars

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..133k&link_type=abstract

Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology ASP Conference Series, Vol. 353, Proceedings of the Confe

Physics

Scientific paper

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.

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