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@inproceedings{702599,
author = {Krtička, Jiří and Kubát, Jiří},
address = {San Francisco, USA},
booktitle = {Stellar Evolution at Low Metallicity: Mass Loss, Explosions},
keywords = {stars: mass-loss - stars: winds outflows -- stars: early-type - stars: circumstellar matter},
language = {eng},
location = {San Francisco, USA},
isbn = {1-58381-221-0},
pages = {133-140},
publisher = {Astronomical Society of the Pacific},
title = {Mass Loss from Massive Zero-Metallicity Stars},
url = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ASPC..353..133K&db_key=AST&data_type=HTML&format=&high=403a2464f518671},
year = {2006}
}
TY - JOUR
ID - 702599
AU - Krtička, Jiří - Kubát, Jiří
PY - 2006
TI - Mass Loss from Massive Zero-Metallicity Stars
PB - Astronomical Society of the Pacific
CY - San Francisco, USA
SN - 1583812210
KW - stars: mass-loss - stars: winds outflows -- stars: early-type - stars: circumstellar matter
UR - http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ASPC..353..133K&db_key=AST&data_type=HTML&format=&high=403a2464f518671
N2 - 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.
ER -
KRTIČKA, Jiří and Jiří KUBÁT. Mass Loss from Massive Zero-Metallicity Stars. In \textit{Stellar Evolution at Low Metallicity: Mass Loss, Explosions}. San Francisco, USA: Astronomical Society of the Pacific, 2006, p.~133-140. ISBN~1-58381-221-0.
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