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@inproceedings{765201,
author = {Krtička, Jiří and Puls, Joachim and Kubát, Jiří},
address = {Potsdam, Germany},
booktitle = {Clumping in hot-star winds},
keywords = {stars: winds; stars: mass-loss; stars: early-type; - hydrodynamics},
language = {eng},
location = {Potsdam, Germany},
isbn = {978-3-940793-33-1},
pages = {111-113},
publisher = {Universität Potsdam},
title = {The influence of clumping on predicted O star wind parameters},
url = {http://opus.kobv.de/ubp/frontdoor.php?source_opus=1796&la=de},
year = {2008}
}
TY - JOUR
ID - 765201
AU - Krtička, Jiří - Puls, Joachim - Kubát, Jiří
PY - 2008
TI - The influence of clumping on predicted O star wind parameters
PB - Universität Potsdam
CY - Potsdam, Germany
SN - 9783940793331
KW - stars: winds
KW - stars: mass-loss
KW - stars: early-type
KW - - hydrodynamics
UR - http://opus.kobv.de/ubp/frontdoor.php?source_opus=1796&la=de
N2 - We study the influence of clumping on the predicted wind structure of O-type stars. For this purpose we artificially include clumping into our stationary wind models. When the clumps are assumed to be optically thin, the radiative line force increases compared to corresponding unclumped models, with a similar effect on either the mass-loss rate or the terminal velocity (depending on the onset of clumping). Optically thick clumps, alternatively, might be able to decrease the radiative force.
ER -
KRTIČKA, Jiří, Joachim PULS a Jiří KUBÁT. The influence of clumping on predicted O star wind parameters. In \textit{Clumping in hot-star winds}. Potsdam, Germany: Universität Potsdam, 2008, s.~111-113. ISBN~978-3-940793-33-1.
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