Evolution state of red giants from seismology

DOI

The detection of oscillations with a mixed character in subgiants and red giants allows us to probe the physical conditions in their cores. With these mixed modes, we aim at determining seismic markers of stellar evolution. Kepler asteroseismic data were selected to map various evolutionary stages and stellar masses. Seismic evolutionary tracks were then drawn with the combination of the frequency and period spacings.

Cone search capability for table J/A+A/572/L5/table1 (Seismic global parameters)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35729005
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/572/L5
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/572/L5
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/572/L5
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/572/L5
Provenance
Creator Mosser B.; Benomar O.; Belkacem K.; Goupil M.J.; Lagarde N.; Michel E.,Lebreton Y.; Stello D.; Vrard M.; Barban C.; Bedding T.R.; Deheuvels S.,Chaplin W.J.; De Ridder J.; Elsworth Y.; Montalban J.; Noels A.,Ouazzani R.M.; Samadi R.; White T.R.; Kjeldsen H.
Publisher CDS
Publication Year 2014
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