Inclusion of Inhomogeneities in Static NLTE Model Atmospheres

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00520211" target="_blank" >RIV/67985815:_____/19:00520211 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Inclusion of Inhomogeneities in Static NLTE Model Atmospheres
Original language description
The presence of inhomogeneities (i.e. clumping) is a generally accepted property of stellar winds. However, in static stellar atmospheres, clumping is usually not considered at all. We describe implementation of clumping to our static NLTE model atmosphere code. We present test results and estimate the effect of clumping on atmospheric structure and emergent radiation.
Czech name
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Czech description
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Project
<a href="/en/project/GA18-05665S" target="_blank" >GA18-05665S: Mass-loss in evolved massive stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Radiative Signatures from the Cosmos: A Conference in Honor of Ivan Hubený
ISBN
9781583819265
ISSN
1050-3390
e-ISSN
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Number of pages
6
Pages from-to
45-50
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Paris
Event date
Oct 23, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000494866300008

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