Non-linear limb-darkening law for LTE models. II. Virtual Observatory Resource

Authors

1. Claret A.

Published by

CDS

Abstract

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.

Keywords

1. Astronomical models
2. Stellar atmospheres
3. Optical astronomy
4. Narrow band photometry
5. Wide-band photometry

Bibliographic source Bibcode

2003A&A...401..657C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/401/657

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/401/657

Document Object Identifer DOI

doi:10.26093/cds/vizier.34010657

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/401/657
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/401/657
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/401/657

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).