Non-linear limb-darkening law for LTE models. II. (Claret, 2003)

Details Non-linear limb-darkening law for LTE models. II. (Claret, 2003) Non-linear limb-darkening law for LTE models. II. (Claret, 2003)

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34010657c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/401/657. Originally published in: 2003A&A...401..657C

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Models: Atmosphere, Photometry: Geneva, Photometry: Vbluw

Scientific paper

As an extension of our previous investigations on stellar atmospheres (Claret, 2000, Cat. ), 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 logg, 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.
(12 data files).

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