Limb-darkening coefficients for ubvyUBVRIJHK (Claret 1998)

Details Limb-darkening coefficients for ubvyUBVRIJHK (Claret 1998) Limb-darkening coefficients for ubvyUBVRIJHK (Claret 1998)

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..33350647c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/335/647. Originally published in: 1998A&A...335..647C

Computer Science

1

Binaries: Eclipsing, Models: Evolutionary

Scientific paper

Linear and non-linear limb-darkening coefficients for the photometric bands u v b y U B V R I J H K are computed for very low effective temperatures stars. The atmosphere models used (PHOENIX-NextGen) do not include the effects of dust formation and dust opacities. These calculations are presented for the first time . The calculations extend the range of effective temperatures (2000K-50000K) covered by our previous papers. These data are important in order to deal with stars in the lower part of Main-Sequence like M or brown dwarfs. The non-linear behavior of the limb-darkening laws, particularly in this effective temperature range, is emphasized and we urge users to take it into account.
(3 data files).

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