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@inproceedings{1480417,
author = {Krtička, Jiří and Kubát, Jiří},
address = {SAN FRANCISCO},
booktitle = {WORKSHOP ON ASTROPHYSICAL OPACITIES},
editor = {Mendoza, C TurckChieze, S Colgan, J},
keywords = {stellar wind; hot star},
howpublished = {tištěná verze "print"},
language = {eng},
location = {SAN FRANCISCO},
pages = {201-206},
publisher = {ASTRONOMICAL SOC PACIFIC},
title = {METUJE Global Hot Star Wind Models},
url = {http://adsabs.harvard.edu/abs/2018ASPC..515..201K},
year = {2018}
}
TY - JOUR
ID - 1480417
AU - Krtička, Jiří - Kubát, Jiří
PY - 2018
TI - METUJE Global Hot Star Wind Models
PB - ASTRONOMICAL SOC PACIFIC
CY - SAN FRANCISCO
KW - stellar wind
KW - hot star
UR - http://adsabs.harvard.edu/abs/2018ASPC..515..201K
N2 - We describe our own global (unified) hydrodynamic models of expanding atmospheres of hot stars. The models solve the hydrodynamic equations, kinetic equilibrium equations (non-LTE), and the comoving-frame radiative transfer equation consistently from the (nearly) hydrostatic photosphere to the supersonic wind. The model input parameters are the stellar effective temperature, radius, mass, and elemental abundances. For these stellar parameters, our code predicts the photosphere and wind structure and, in particular, the wind mass -loss rate and terminal velocity. The photospheric emergent flux and thermal structure nicely agree with the TLUSTY model atmospheres.
ER -
KRTIČKA, Jiří a Jiří KUBÁT. METUJE Global Hot Star Wind Models. Online. In Mendoza, C TurckChieze, S Colgan, J. \textit{WORKSHOP ON ASTROPHYSICAL OPACITIES}. SAN FRANCISCO: ASTRONOMICAL SOC PACIFIC, 2018. s.~201-206. ISSN~1050-3390. [citováno 2024-04-24]
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