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Non-LTE Line Formation for Trace Elements in Stellar Atmospheres
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http://hub.abes.fr/edp/periodical/eas/2010/volume_43
Title
Non-LTE Line Formation for Trace Elements in Stellar Atmospheres
has manifestation of work
http://hub.abes.fr/edp/periodical/eas/2010/volume_43/issue_2010/m/print
http://hub.abes.fr/edp/periodical/eas/2010/volume_43/issue_2010/m/web
publisher identifier
eas/2010/04
is
Is Part Of
of
Radiative Transfer in Stellar Atmospheres
Background Opacities
Foreword
NLTE analysis of spectra i: Departures from LTE for A-type stars
Mechanisms of departure from lte
Non-LTE Line Formation in the Near-IR: Hot Stars
Radiative Transfer Methods: new exact results for testing the accuracy of the ALI numerical method for a stellar atmosphere
An Introduction to the Subject of this Workshop
Atomic Data
Accurate Collisional Cross-Sections: Important Non-Lte Input Data
Oscillator Stengths and Their Uncertainties
On the Properties of B and A Type Supergiants
Departures from lte in chemically stratified atmospheres
Statistical equilibrium equations for trace elements in stellar atmospheres
Non-LTE Model Atom Construction
Resonance broadening and van der waals broadening
Stark Broadening
Atmospheric parameter determination for massive stars via non-LTE spectrum analysis
Departures from LTE in Cool Stars
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