Effective temperatures and spectral energy distribution for A and F stars in the near infrared - Comparison with theoretical models

Details Effective temperatures and spectral energy distribution for A and F stars in the near infrared - Comparison with theoretical models Effective temperatures and spectral energy distribution for A and F stars in the near infrared - Comparison with theoretical models

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..528g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, May-June 1990, p. 528-535. In Russian.

Astronomy and Astrophysics

Astronomy

3

A Stars, Energy Distribution, F Stars, Near Infrared Radiation, Stellar Spectra, Stellar Temperature, Infrared Astronomy, Spectrophotometry, Stellar Luminosity

Scientific paper

The observed energy distribution for A and F stars is compared with theoretical model atmospheres of Kurucz in the 6000-10,800 A range. A and F stars of the IV and V luminosity classes are shown to have IR excesses of about 5-6 percent in the 8000-10,800 A region. IR excesses of A and F giants and rapidly rotating stars with v sin i greater than 300 km/s are 9-11 percent.

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