Comparison of theoretical model atmospheres of VEGA with results of observations

Details Comparison of theoretical model atmospheres of VEGA with results of observations Comparison of theoretical model atmospheres of VEGA with results of observations

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1....3t&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, Sept.-Oct. 1985, p. 3-9. In Russian.

Physics

A Stars, Stellar Atmospheres, Stellar Models, Stellar Spectrophotometry, Far Infrared Radiation, Stellar Envelopes

Scientific paper

The main model atmospheres of Vega are described, and it is shown that
the best agreement with experimental results is obtained for the model
atmosphere with the parameters Teff = 9570 K and log g = 3.95. The large
radiation excess in the far infrared is shown to be caused by a dusty
shell around Vega.

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