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@inproceedings{806161,
author = {Krtička, Jiří and Muijres, Lianne and Puls, Joachim and Kubát, Jiří and de Koter, Alex},
address = {Cambridge, United Kingdom},
booktitle = {The Art of Modelling Stars in the 21st Century},
keywords = {stars: winds; outflows stars: mass-loss; stars: early-type; hydrodynamics},
language = {eng},
location = {Cambridge, United Kingdom},
isbn = {978-0-521-88983-4},
pages = {283-286},
publisher = {Cambridge University Press},
title = {The influence of inhomogeneities on hot star wind model predictions},
url = {http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=2451852},
year = {2008}
}
TY - JOUR
ID - 806161
AU - Krtička, Jiří - Muijres, Lianne - Puls, Joachim - Kubát, Jiří - de Koter, Alex
PY - 2008
TI - The influence of inhomogeneities on hot star wind model predictions
PB - Cambridge University Press
CY - Cambridge, United Kingdom
SN - 9780521889834
KW - stars: winds
KW - outflows stars: mass-loss
KW - stars: early-type
KW - hydrodynamics
UR - http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=2451852
N2 - We study the effect of wind inhomogeneities (clumping) on O star wind model predictions. For this purpose we artificially include clumping into our stationary NLTE wind models. As a result of the inclusion of optically thin clumps the radiative line force is increased compared to corresponding unclumped models, with a similar effect on either the mass-loss rate or the terminal velocity. When the clumps are allowed to be optically thick in continuum, on the other hand, the radiative force and consequently the mass-loss rate decreases alternatively.
ER -
KRTIČKA, Jiří, Lianne MUIJRES, Joachim PULS, Jiří KUBÁT and Alex DE KOTER. The influence of inhomogeneities on hot star wind model predictions. In \textit{The Art of Modelling Stars in the 21st Century}. Cambridge, United Kingdom: Cambridge University Press, 2008, p.~283-286. ISBN~978-0-521-88983-4.
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