A new non-linear limb-darkening law for LTE stellar atmosphere models II K at several surface gravities. Geneva and Walraven systems: Calculations for -5.0 <= log [M/H] <= +1 2000 K <= Teff <= 50,000 K at several surface gravities

Details A new non-linear limb-darkening law for LTE stellar atmosphere models II K at several surface gravities. Geneva and Walraven systems: Calculations for -5.0 <= log [M/H] <= +1 2000 K <= Teff <= 50,000 K at several surface gravities A new non-linear limb-darkening law for LTE stellar atmosphere models II K at several surface gravities. Geneva and Walraven systems: Calculations for -5.0 <= log [M/H] <= +1 2000 K <= Teff <= 50,000 K at several surface gravities

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...401..657c&link_type=abstract

Astronomy and Astrophysics, v.401, p.657-660 (2003)

Astronomy and Astrophysics

Astrophysics

18

Stars: Atmospheres, Stars: Binaries: Eclipsing, Stars: Abundances

Scientific paper

As an extension of our previous investigations on stellar atmospheres (Claret \cite{Claret00}), 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, T_eff, 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.
Tables 2-38 are available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/401/657. Additional data are available on CD ROMs upon request.

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