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@inproceedings{806579,
author = {Kraus, Michaela and Kubát, Jiří and Krtička, 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 = {51-53},
publisher = {Universität Potsdam},
title = {Wind emission of OB supergiants and the influence of clumping},
url = {http://opus.kobv.de/ubp/frontdoor.php?source_opus=1796&la=de},
year = {2008}
}
TY - JOUR
ID - 806579
AU - Kraus, Michaela - Kubát, Jiří - Krtička, Jiří
PY - 2008
TI - Wind emission of OB supergiants and the influence of clumping
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 - The influence of the wind to the total continuum of OB supergiants is discussed. For wind velocity distributions with beta > 1.0, the wind can have strong influence to the total continuum emission, even at optical wavelengths. Comparing the continuum emission of clumped and unclumped winds, especially for stars with high beta values, delivers flux differences of up to 30% with maximum in the near-IR. Continuum observations at these wavelengths are therefore an ideal tool to discriminate between clumped and unclumped winds of OB supergiants.
ER -
KRAUS, Michaela, Jiří KUBÁT a Jiří KRTIČKA. Wind emission of OB supergiants and the influence of clumping. In \textit{Clumping in hot-star winds}. Potsdam, Germany: Universität Potsdam, 2008, s.~51-53. ISBN~978-3-940793-33-1.
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