The gravity-brightening effect and stellar atmospheres. I. Results for models with 3700K<T_eff_<7000K.

Details The gravity-brightening effect and stellar atmospheres. I. Results for models with 3700K<T_eff_<7000K. The gravity-brightening effect and stellar atmospheres. I. Results for models with 3700K<T_eff_<7000K.

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...326..257a&link_type=abstract

Astronomy and Astrophysics, v.326, p.257-262

Astronomy and Astrophysics

Astrophysics

18

Atmospheres, Stars: Binaries: Close, Stars: Binaries: Eclipsing, Stars: Fundamental Parameters, Stars: General

Scientific paper

The gravity-brightening exponent (β) is studied using the UMA (Uppsala Model Atmosphere) code in non-illuminated convective grey (in the sense of ``continuum only'' opacity) and non-grey (line blanketed) atmospheres, for 3700K

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