Structure and evolution of low-mass stars

DOI

Properties of Very Low mass stars for different initial metallicity [M/H] and Helium mass fraction: mass (in solar mass), age (in Gyrs) effective temperature (in K), log of luminosity (in solar L), radius (10^10cm), central temperature Tc (in K) and density RHOc (in gr/cm-3). Abundances of light elements are normalised to their initial abundance (see text).

Identifier
DOI http://doi.org/10.26093/cds/vizier.33271039
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/327/1039
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/327/1039
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/327/1039
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/327/1039
Provenance
Creator Chabrier G.; Baraffe I.
Publisher CDS
Publication Year 1997
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; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy