STAGGER-grid of 3D stellar models. V. Virtual Observatory Resource

Authors

1. Chiavassa A.
2. Casagrande L.
3. Collet R.
4. Magic Z.
5. Bigot L.
6. Thevenin F.,Asplund M.

Published by

CDS

Abstract

We have calculated spectra from 1000 to 200000{AA} with a constant resolving power of {lambda}/{Delta}{lambda}=20000 and from 8470 and 8710{AA} (Gaia Radial Velocity Spectrometer - RVS - spectral range) with a constant resolving power of {lambda}/{Delta}{lambda}=300000. This for the Stagger-grid 3D stellar atmosphere models in the ranges: Teff from 4000 to 7000K, logg from 1.5 to 5.0, and [Fe/H], from -4.0 to +0.5. We used synthetic spectra to compute theoretical colours in the Johnson-Cousins UBV(RI)C, SDSS, 2MASS, Gaia, SkyMap- per, Stroemgren systems, and HST-WFC3.

Keywords

1. astronomical-models
2. stellar-atmospheres
3. late-type-stars
4. two-color-diagrams
5. radial-velocity

Bibliographic source Bibcode

2018A&A...611A..11C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/611/A11

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/611/A11

Document Object Identifer DOI

doi:10.26093/cds/vizier.36110011

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