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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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