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@inproceedings{702602,
author = {Krtička, Jiří and Kubát, Jiří},
address = {Paříž, Francie},
booktitle = {The Universe at z 〉 6, 26th meeting of the IAU, Joint Discussion 7},
keywords = {stars: mass-loss - stars: winds outflows -- stars: early-type - stars: circumstellar matter},
language = {eng},
location = {Paříž, Francie},
isbn = {123456789012345},
pages = {26-26},
publisher = {International Astronomical Union},
title = {The mass loss from hot Pop III stars},
url = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006IAUJD...7E..26K&db_key=AST&data_type=HTML&format=&high=403a2464f518671},
year = {2006}
}
TY - JOUR
ID - 702602
AU - Krtička, Jiří - Kubát, Jiří
PY - 2006
TI - The mass loss from hot Pop III stars
PB - International Astronomical Union
CY - Paříž, Francie
SN - 123456789012345
KW - stars: mass-loss - stars: winds outflows -- stars: early-type - stars: circumstellar matter
UR - http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006IAUJD...7E..26K&db_key=AST&data_type=HTML&format=&high=403a2464f518671
N2 - We test the possibility of the line and continuum driven wind from hot zero-metallicity Pop III stars. For this purpose we apply our own NLTE wind model and test the possibility of wind existence for zero-metallicity Pop III stars with parameters corresponding to the zero-age main sequence. Because hydrogen and helium are highly ionized and do not have enough lines to drive the stellar wind, the line-driven winds from hot very massive zero-metallicity stars are unlikely. The expulsion of individual atoms or ions is also either unlikely or negligible. We discuss the implications of these results on the evolution of Pop III stars and possible other mechanisms of mass-loss from these stars and for the models of the reionization of the Universe.
ER -
KRTIČKA, Jiří a Jiří KUBÁT. The mass loss from hot Pop III stars. In \textit{The Universe at z 〉 6, 26th meeting of the IAU, Joint Discussion 7}. Paříž, Francie: International Astronomical Union, 2006, s.~26-26. ISBN~123456789012345.
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