TY  - JOUR
A1  - Votruba, Viktor
A1  - Feldmeier, Achim
A1  - Krticka, Jiri
A1  - Kubát, Jiří
T1  - Multicomponent stellar wind from hot subdwarfs stars
N2  - Stellar wind from hot subdwarf stars is mainly accelerated by the interaction of ultraviolet photospheric radiation with metals, mainly oxygen. Absorbing ions share momentum through Coulombic collisions with the remaining passive part of the plasma (namely protons). We found that in the case of the winds from hot subdwarfs, interactions could be so small that they stop the momentum transfer between the passive bulk of plasma and absorbing ions. As a result wind decouples at a certain point.
Y1  - 2010
UR  - http://www.springerlink.com/content/100241
U6  - https://doi.org/10.1007/s10509-010-0402-2
SN  - 0004-640X
ER  -