Instabilities in radiation driven stellar winds.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F03%3A01030166" target="_blank" >RIV/67985815:_____/03:01030166 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Instabilities in radiation driven stellar winds.
Original language description
The Rayleigh-Taylor type instability in a radiatively driven stellar wind is analyzed.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2003
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Stellar atmosphere modeling.
ISBN
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ISSN
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e-ISSN
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Number of pages
4
Pages from-to
263-266
Publisher name
Astronomical Society of Pacific
Place of publication
San Francisco
Event location
Tubingen [DE]
Event date
Apr 8, 2002
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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