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@inproceedings{568599,
author = {Krtička, Jiří and Kubát, Jiří},
address = {Cambridge},
booktitle = {Proceedings of the IAUS224: The A-Star Puzzle},
keywords = {stars: atmospheres -- stars: early-type --stars: winds; outflows --radiative transfer},
language = {eng},
location = {Cambridge},
isbn = {0521850185},
pages = {23-28},
publisher = {Cambridge University Press},
title = {NLTE wind models of A supergiants},
url = {http://journals.cambridge.org/bin/bladerunner?REQUNIQ=1109866025&REQSESS=2521642&118000REQEVENT=&REQINT1=280604&REQAUTH=0},
year = {2005}
}
TY - JOUR
ID - 568599
AU - Krtička, Jiří - Kubát, Jiří
PY - 2005
TI - NLTE wind models of A supergiants
PB - Cambridge University Press
CY - Cambridge
SN - 0521850185
KW - stars: atmospheres -- stars: early-type --stars: winds
KW - outflows --radiative transfer
UR - http://journals.cambridge.org/bin/bladerunner?REQUNIQ=1109866025&REQSESS=2521642&118000REQEVENT=&REQINT1=280604&REQAUTH=0
N2 - We present new numerical models of line-driven stellar winds of A supergiants. Statistical equilibrium (NLTE) equations of the most abundant elements are solved, and properly obtained occupation numbers are used to calculate consistent radiative force and radiative heating terms. Wind density, velocity, and temperature are calculated as a solution of model hydrodynamical equations. Our models allow for the calculation of wind mass-loss rate and terminal velocity.
ER -
KRTIČKA, Jiří a Jiří KUBÁT. NLTE wind models of A supergiants. In \textit{Proceedings of the IAUS224: The A-Star Puzzle}. Cambridge: Cambridge University Press, 2005, s.~23-28. ISBN~0521850185.
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