| KRTIČKA, Jiří, Stanley P. OWOCKI, Jiří KUBÁT, Ross K. GALLOWAY and John C. BROWN. On multicomponent effects in stellar winds of stars at extremely low metallicity. Astronomy and Astrophysics. Les Ulis Cedex, France: EDP Sciences, 2003, vol. 35, No 402, p. 713-718. ISSN 0004-6361. |
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@article{486041,
author = {Krtička, Jiří and Owocki, Stanley P. and Kubát, Jiří and Galloway, Ross K. and Brown, John C.},
article_location = {Les Ulis Cedex, France},
article_number = {402},
keywords = {stars: mass-loss -- stars: early-type -- stars:abundances -- stars: winds; outflows},
language = {eng},
issn = {0004-6361},
journal = {Astronomy and Astrophysics},
title = {On multicomponent effects in stellar winds of stars at extremely low metallicity},
url = {http://www.edpsciences.org/articles/aa/abs/2003/17/aah4143/aah4143.html},
volume = {35},
year = {2003}
}
TY - JOUR
ID - 486041
AU - Krtička, Jiří - Owocki, Stanley P. - Kubát, Jiří - Galloway, Ross K. - Brown, John C.
PY - 2003
TI - On multicomponent effects in stellar winds of stars at extremely low metallicity
JF - Astronomy and Astrophysics
VL - 35
IS - 402
SP - 713-718
EP - 713-718
PB - EDP Sciences
SN - 00046361
KW - stars: mass-loss -- stars: early-type -- stars:abundances -- stars: winds
KW - outflows
UR - http://www.edpsciences.org/articles/aa/abs/2003/17/aah4143/aah4143.html
N2 - We calculate multicomponent line-driven wind models of stars at extremely low metallicity suitable for massive first generation stars. For most of the models we find that the multicomponent wind nature is not important for either wind dynamics or for wind temperature stratification. However, for stars with the lowest metallicities we find that multicomponent effects influence the wind structure. These effects range from pure heating to possible fallback of the nonabsorbing wind component. We present a simple formula for the calculation of metallicity for which the multicomponent effects become important. We show that the importance of the multicomponent nature of winds of low metallicity stars is characterised not only by the low density of driving ions, but also by lower mass-loss rate.
ER -
KRTIČKA, Jiří, Stanley P. OWOCKI, Jiří KUBÁT, Ross K. GALLOWAY and John C. BROWN. On multicomponent effects in stellar winds of stars at extremely low metallicity. \textit{Astronomy and Astrophysics}. Les Ulis Cedex, France: EDP Sciences, 2003, vol.~35, No~402, p.~713-718. ISSN~0004-6361.
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