Modelling of AGB stars in the LMC

DOI

Asymptotic giant branch (AGB) stars are major contributors to both the chemical enrichment of the interstellar medium and the integrated light of galaxies. Despite its importance, the AGB is one of the least understood phases of stellar evolution. The main difficulties associated with detailed modelling of the AGB are related to the mass-loss process and the 3rd dredge-up efficiency. We provide direct measures of mass-loss rates and luminosities for a complete sample of AGB stars in the Large Magellanic Cloud, disentangling the C- and O-rich stellar populations.

Cone search capability for table J/A+A/537/A105/results (Parameters of best-fitting models for all AGB candidates (table2))

Identifier
DOI http://doi.org/10.26093/cds/vizier.35370105
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/537/A105
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/537/A105
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/537/A105
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/537/A105
Provenance
Creator Gullieuszik M.; Groenewegen M.A.T.; Cioni M.-R.L.; de Grijs R.,van Loon J.T.; Girardi L.; Ivanov V.D.; Oliveira J.M.; Emerson J.P.,Guandalini R.
Publisher CDS
Publication Year 2012
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