Basics of the NLTE Physics
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00440280" target="_blank" >RIV/67985815:_____/14:00440280 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/978-3-319-06956-2_14" target="_blank" >http://dx.doi.org/10.1007/978-3-319-06956-2_14</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/978-3-319-06956-2_14" target="_blank" >10.1007/978-3-319-06956-2_14</a>
Alternative languages
Result language
angličtina
Original language name
Basics of the NLTE Physics
Original language description
The basic assumptions of the NLTE approximation in stellar atmospheres are summarized. The assumptions of thermodynamic equilibrium, local thermodynamic equilibrium (LTE), and non-LTE (NLTE) are compared. It is emphasized that LTE is a poor approximation if radiative transitions dominate in stellar atmospheres. The equations of kinetic equilibrium and methods of their solution are discussed.
Czech name
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Czech description
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Classification
Type
C - Chapter in a specialist book
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA13-10589S" target="_blank" >GA13-10589S: Mass loss in hot massive stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Book/collection name
Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars
ISBN
978-3-319-06955-5
Number of pages of the result
9
Pages from-to
149-157
Number of pages of the book
310
Publisher name
Springer
Place of publication
Heidelberg
UT code for WoS chapter
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