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Power-2 limb-darkening coefficients for the , , SDSS , Gaia, Kepler, TESS, and CHEOPS photometric systems II. PHOENIX spherically symmetric stellar atmosphere models
A. Claret, J. Southworth
Multiple parametric limb-darkening laws have been presented, and there are many available sources of theoretical limb-darkening coefficients (LDCs) calculated using stellar model a…
Theoretical tidal evolution constants for stellar models from the pre-main sequence to the white dwarf stage Apsidal motion constants, moment of inertia, and gravitational potential energy
A. Claret
One of the most reliable means of studying the stellar interior is through the apsidal motion in double line eclipsing binary systems since these systems present errors in masses,…
Power-2 limb-darkening coefficients for the uvby, UBVRIJHK, SDSS ugriz, Gaia, Kepler, and TESS photometric systems
A. Claret, J. Southworth
Limb darkening is an important stellar phenomenon and must be accounted for in the study of stellar spectra, eclipsing binaries, transiting planetary systems, and microlensing even…
Exploratory scenarios for the differential nuclear and tidal evolution of TZ Fornacis
A. Claret
TZ Fornacis is a double-lined eclipsing binary system with similar masses (2.0570.001 and 1.9580.001 ) but characterized by very different radii (8.280.22…