SI II, III and IV in non-LTE for temperature determination in B-stars

Details SI II, III and IV in non-LTE for temperature determination in B-stars SI II, III and IV in non-LTE for temperature determination in B-stars

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...235..326b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 235, no. 1-2, Aug. 1990, p. 326-334.

Physics

87

B Stars, Nonequilibrium Thermodynamics, Silicon, Stellar Spectra, Stellar Temperature, Line Spectra, Plasma Diagnostics, Stellar Atmospheres, Stellar Models, Stellar Physics

Scientific paper

A non-LTE line formation calculation for Si II, III and IV is presented.
The model atom is described and its application to temperature
determination in B-stars is discussed.

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