Multicomponent stellar wind from hot subdwarfs stars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F10%3A00049014" target="_blank" >RIV/00216224:14310/10:00049014 - isvavai.cz</a>
Alternative codes found
RIV/67985815:_____/10:00354882
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Multicomponent stellar wind from hot subdwarfs stars
Original language description
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.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GP205%2F09%2FP476" target="_blank" >GP205/09/P476: Dynamics of multicomponent stellar wind from hot stars</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysics and Space Science
ISSN
0004-640X
e-ISSN
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Volume of the periodical
329
Issue of the periodical within the volume
1
Country of publishing house
DE - GERMANY
Number of pages
3
Pages from-to
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UT code for WoS article
000282823200026
EID of the result in the Scopus database
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