Modelling of Magellanic Cloud C/O stars

DOI

Mass loss is one of the fundamental properties of Asymptotic Giant Branch (AGB) stars, and through the enrichment of the interstellar medium, AGB stars are key players in the life cycle of dust and gas in the universe. However, a quantitative understanding of the mass-loss process is still largely lacking, particularly its dependence on metallicity. To investigate the relation between mass loss, luminosity and pulsation period for a large sample of evolved stars in the Small and Large Magellanic Cloud.

Cone search capability for table J/A+A/506/1277/Cstars (C-star sample: identifiers, pulsation periods, and fit results)

Cone search capability for table J/A+A/506/1277/table2o (O-star sample: identifiers and pulsation periods)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35061277
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/506/1277
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/506/1277
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/506/1277
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/506/1277
Provenance
Creator Groenewegen M.A.T.; Sloan G.C.; Soszynski I.; Petersen E.A.
Publisher CDS
Publication Year 2009
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; Galactic and extragalactic Astronomy; Natural Sciences; Physics; Stellar Astronomy