2013A&A...552A..16C


C.D.S. - SIMBAD4 rel 1.7 - 2020.08.09CEST02:13:35

2013A&A...552A..16C - Astronomy and Astrophysics, volume 552A, 16-16 (2013/4-1)

New limb-darkening coefficients for Phoenix/1d model atmospheres. II. Calculations for 5000 K ≤ teff ≤ 10000 K Kepler, CoRot, Spitzer, uvby, UBVRIJHK, Sloan, and 2MASS photometric systems.

CLARET A., HAUSCHILDT P.H. and WITTE S.

Abstract (from CDS):

We present an extension of our investigations on limb-darkening coefficients computed with spherical symmetrical Phoenix models. The models investigated in this paper cover the range 5000K≤Teff≤10000K and complete our previous studies of low effective temperatures computed with the same code. The limb-darkening coefficients are computed for the transmission curves of the Kepler, CoRoT, and Spitzer space missions and the Stroemgren, Johnson-Cousins, Sloan, and 2MASS passbands. These computations were performed by adopting the least-squares method. We have used six laws to describe the specific intensity distribution: linear, quadratic, square root, logarithmic, exponential, and a general law with four terms. The computations are presented for the solar chemical composition and cover the range 3.0≤logg≤5.5. The adopted microturbulent velocity and the mixing-length parameter are 2.0km/s and 2.0.

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Journal keyword(s): stars: atmospheres - binaries: eclipsing - planetary systems

VizieR on-line data: <Available at CDS (J/A+A/552/A16): tableu.dat mu.dat tableab.dat mab.dat tablecd.dat mcd.dat tableef.dat mef.dat tablegh.dat mgh.dat tableghs.dat mghs.dat tablee6.dat meq6.dat tablee6s.dat meq6s.dat>

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2020.08.09-02:13:35

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