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@inproceedings{572437,
author = {Krtička, Jiří and Kubát, Jiří},
address = {Nižnyj Archyz, Rusko},
booktitle = {Magnetic stars},
keywords = {hydrodynamics -- stars: mass-loss -- stars: winds -- stars: chemically peculiar},
language = {eng},
location = {Nižnyj Archyz, Rusko},
pages = {234-240},
publisher = {SAO RAS},
title = {Multicomponent stellar winds of He chemically peculiar stars},
url = {http://xxx.lanl.gov/abs/astro-ph/0310751},
year = {2004}
}
TY - JOUR
ID - 572437
AU - Krtička, Jiří - Kubát, Jiří
PY - 2004
TI - Multicomponent stellar winds of He chemically peculiar stars
PB - SAO RAS
CY - Nižnyj Archyz, Rusko
KW - hydrodynamics -- stars: mass-loss -- stars: winds -- stars: chemically peculiar
UR - http://xxx.lanl.gov/abs/astro-ph/0310751
N2 - We calculate multicomponent stellar wind models with inclusion of a helium component applicable to He-rich and He-poor stars. We show that helium does not decouple from the stellar wind of He-rich stars due to its coupling to hydrogen and its ionized state. For He-poor stars helium may decouple from the stellar wind, however this effect is not able to explain the chemical peculiarity of these stars. We conclude that the explanation of chemical peculiarity of these stars based purely on helium or hydrogen decoupling from the stellar wind is unlikely.
ER -
KRTIČKA, Jiří a Jiří KUBÁT. Multicomponent stellar winds of He chemically peculiar stars. In \textit{Magnetic stars}. Nižnyj Archyz, Rusko: SAO RAS. s.~234-240. 2004.
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