Limb-darkening for cool stars - Standard and irradiated models

Details Limb-darkening for cool stars - Standard and irradiated models Limb-darkening for cool stars - Standard and irradiated models

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169..223c&link_type=abstract

(IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics a

Astronomy and Astrophysics

Astrophysics

1

Atmospheric Models, Binary Stars, Cool Stars, Limb Darkening, Thermodynamic Equilibrium, Angular Distribution, Companion Stars, Giant Stars, Least Squares Method, Main Sequence Stars, Stellar Temperature

Scientific paper

Limb-darkening coefficients for a grid of nongrey LTE atmosphere models
has been calculated by means of Upsalla Model Atmosphere code using a
least-squares fitting. Both linear and quadratic laws were adopted in
the standard models and in those with irradiation from a companion star
as well, which is more realistic for the case of close binaries.

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