Abundance study of LMC post-AGB stars

DOI

The photospheric abundances of evolved solar-type stars of different metallicities serve as probes into stellar evolution theory. Stellar photospheres of post-asymptotic giant branch (post-AGB) stars bear witness to the internal chemical enrichment processes, integrated over their entire stellar evolution. Here we study post-AGB stars in the Large Magellanic Cloud (LMC). With their known distances, these rare objects are ideal tracers of AGB nucleosynthesis and dredge-up phenomena.

Cone search capability for table J/A+A/554/A106/stars (Stars summary (added at CDS))

Identifier
DOI http://doi.org/10.26093/cds/vizier.35540106
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/554/A106
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/554/A106
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/554/A106
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/554/A106
Provenance
Creator van Aarle E.; Van Winckel H.; De Smedt K.; Kamath D.; Wood P.R.
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; Galactic and extragalactic Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics