Grid of 1D models for Mg line formation Virtual Observatory Resource

Authors

1. Osorio Y.
2. Barklem P.S.

Published by

CDS

Abstract

Mg is the alpha element of choice for Galactic population and chemical evolution studies as it is easily detectable in all late-type stars. Such studies require precise elemental abundances, and thus departures from LTE need to be accounted for.

Keywords

1. astronomical-models
2. stellar-atmospheres
3. chemical-abundances
4. line-intensities

Bibliographic source Bibcode

2016A&A...586A.120O

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/586/A120

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/586/A120

Document Object Identifer DOI

doi:10.26093/cds/vizier.35860120

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/586/A120
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/586/A120
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/586/A120

IVOA Table Access TAP

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