Linearized limb-darkening coefficients for use in analysis of eclipsing binary light curves

Details Linearized limb-darkening coefficients for use in analysis of eclipsing binary light curves Linearized limb-darkening coefficients for use in analysis of eclipsing binary light curves

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..53..181a&link_type=abstract

Astrophysics and Space Science, vol. 53, no. 1, Jan. 1978, p. 181-192.

Astronomy and Astrophysics

Astrophysics

360

Eclipsing Binary Stars, Light Curve, Limb Darkening, Stellar Atmospheres, Stellar Radiation, Coefficients, Curve Fitting, Infrared Spectra, Monochromatic Radiation, Stellar Temperature

Scientific paper

Monochromatic limb-darkening coefficients are derived from a linear limb-darkening law; the coefficients are suitable for the interpretation of eclipsing binary light curves. Coefficients for effective temperatures between 50,000 and 4000 C, wavelengths between 0.2 and 2.2 microns, and a range of gravity values are presented. Comparison of the theoretical values with empirically determined coefficients shows a better agreement between theory and observation than previously obtained.

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