Comparison between LTE and non-LTE abundances from the analysis of stellar atmospheres

Details Comparison between LTE and non-LTE abundances from the analysis of stellar atmospheres Comparison between LTE and non-LTE abundances from the analysis of stellar atmospheres

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....37..117f&link_type=abstract

Astronomy and Astrophysics, vol. 37, no. 1, Dec. 1974, p. 117-120. Translation.

Astronomy and Astrophysics

Astrophysics

9

Abundance, Line Spectra, Stellar Atmospheres, Stellar Spectra, Thermodynamic Equilibrium, Astronomical Models, Atmospheric Composition, Atmospheric Ionization, Optical Thickness, Photoionization, Spectrum Analysis

Scientific paper

The present work analyzes the direction of the non-LTE effects both on
the source function and on the optical depth in a line, and their
influence on abundance determination. Deviations, relative to the LTE
values, exhibited by the abundances one would obtain from the analysis
of given data, are systematically presented.

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