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Linear and Non-Linear Limb Darkening Coefficients for Synthetic Light Curve Modeling of Binary Stars

  • J. Díaz-Cordovés
  • A. Claret
  • A. Giménez
Conference paper

Abstract

Linear and quadratic limb darkening coefficients have been calculated by means of a least squares fitting for a large sample of stellar model atmospheres. A range in temperatures from 4000 to 50000 K has been covered from the zero-age main sequence up to the giant phases. A new law for the limb-darkening of hot stars, based on a square-root term, is also included. The validity of the different approximations for the analysis of light curves of eclipsing binaries is discussed.

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References

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Copyright information

© Springer-Verlag New York, Inc. 1993

Authors and Affiliations

  • J. Díaz-Cordovés
    • 1
  • A. Claret
    • 2
  • A. Giménez
    • 3
  1. 1.Instituto “Alvaro de Mendaña”Ponferrada (León)Spain
  2. 2.Instituto de Astrofísica de AndalucíaGranadaSpain
  3. 3.Laboratorio de Astrofísica Espacial y Física FundamentalEstación de Villafranca del CastilloMadridSpain

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