NLTE formation of oxygen lines in irradiated stellar atmospheres.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F03%3A01030171" target="_blank" >RIV/67985815:_____/03:01030171 - 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
NLTE formation of oxygen lines in irradiated stellar atmospheres.
Original language description
NLTE model stellar atmopheres are calculated under the assumption of hydrostatic and radiative equilibrium using the computer code ATA. The atmospheres are assumed to be irradiated by an external source of ratiation.
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
Modelling of stellar atmospheres.
ISBN
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ISSN
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e-ISSN
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Number of pages
1
Pages from-to
"B6"
Publisher name
Astronomical Society of Pacific
Place of publication
San Francisco
Event location
Uppsala [SE]
Event date
Jun 17, 2002
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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