Ages and [Fe/H] of M31 globular clusters

DOI

The formation and evolution of disk galaxies are long standing questions in Astronomy. Understanding the properties of globular cluster systems can lead to important insights on the evolution of its host galaxy. We aim to obtain the stellar population parameters - age and metallicity - of a sample of M31 and Galactic globular clusters. Studying their globular cluster systems is an important step towards understanding their formation and evolution in a complete way.

Cone search capability for table J/A+A/549/A60/M31glcl (Ages and metallicities derived for M31 globular clusters)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35490060
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/549/A60
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/549/A60
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/549/A60
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/549/A60
Provenance
Creator Cezario E.; Coelho P.R.T.; Alves-Brito A.; Forbes D.A.; Brodie J.P.
Publisher CDS
Publication Year 2013
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; Physics; Stellar Astronomy