Volume 401, Number 2, April II 2003
|Page(s)||657 - 660|
|Published online||21 March 2003|
A new non-linear limb-darkening law for LTE stellar atmosphere models II*
Geneva and Walraven systems: Calculations for , 2000 K K at several surface gravities
Instituto de Astrofísica de Andalucía, CSIC, Apartado 3004, 18080 Granada, Spain
Corresponding author: email@example.com
Accepted: 15 January 2003
As an extension of our previous investigations on stellar atmospheres (Claret [CITE]), the limb-darkening coefficients for the Geneva and Walraven photometric systems are presented for the first time using the ATLAS and PHOENIX models. They cover a wide range of values of log g, Teff, metallicities and microturbulent velocities. In addition to the traditional applications of limb-darkening coefficients, the present ones are now being used in the interpretation of phase shift of B and A-F type pulsating stars.
Key words: stars: atmospheres / stars: binaries: eclipsing / stars: abundances
© ESO, 2003
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