Non-linear limb-darkening law for LTE models. II.

DOI

As an extension of our previous investigations on stellar atmospheres (Claret, 2000, Cat. ), 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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34010657
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/401/657
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/401/657
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/401/657
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/401/657
Provenance
Creator Claret A.
Publisher CDS
Publication Year 2003
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy