2024-03-29T09:47:27Zivo://CDS.VizieR/J/A+A/401/6572022-10-10T00:00:00ZJ.A_AIVOANon-linear limb-darkening law for LTE models. II.As an extension of our previous investigations on stellar atmospheres (Claret, 2000, Cat. <J/A+A/363/1081>), the limb-darkening coefficients for the Geneva and Walraven photometric systems are presented for the first time using the ATLAS and PHOENIX models. They cover a wide range of values of logg, T_eff_, metallicities and microturbulent velocities. In addition to the traditional applications of limb-darkening coefficients, the present ones are now being used in the interpretation of phase shift of B and A-F type pulsating stars.Astronomical modelsStellar atmospheresOptical astronomyNarrow band photometryWide-band photometryobservational-astronomystellar-astronomyhttps://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/401/657http://doi.org/10.26093/cds/vizier.34010657https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/401/6572003A&A...401..657Chttp://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/401/657Claret A.CDS2003https://cds.unistra.fr/vizier-org/licences_vizier.htmlCDS support team <cds-question@unistra.fr>DatasetAstroObjectsastronomy