Metallicity of M dwarfs. III. Virtual Observatory Resource

Authors
  1. Neves V.
  2. Bonfils X.
  3. Santos N.C.
  4. Delfosse X.
  5. Forveille T.
  6. Allard F.,Udry S.
  7. Published by
    CDS
Abstract

The aim of this work is the study of the planet-metallicity and the planet-stellar mass correlations for M dwarfs from the HARPS GTO M dwarf subsample. We use a new method that takes advantage of the HARPS high-resolution spectra to increase the precision of metallicity, using previous photometric calibrations of [Fe/H] and effective temperature as starting values.

Keywords
  1. late-type-stars
  2. m-stars
  3. chemical-abundances
Bibliographic source Bibcode
2013A&A...551A..36N
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/551/A36
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/551/A36
Document Object Identifer DOI
doi:10.26093/cds/vizier.35510036

Access

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History

2013-08-23T08:48:24Z
Resource record created
2013-08-23T08:48:24Z
Created
2025-08-05T12:17:05Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr