Ages of SMC young clusters and field stars

DOI

In this paper we discuss the cluster and field star formation in the central part of the Small Magellanic Cloud. The main goal is to study the correlation between young objects and their interstellar environment. The ages of about 164 associations and 311 clusters younger than 1Gyr are determined using isochrone fitting. The spatial distribution of the clusters is compared with the HI maps, with the HI velocity dispersion field, with the location of the CO clouds and with the distribution of young field stars.

Cone search capability for table J/A+A/452/179/table2 (Age and reddening determination for 462 clusters and associations in the SMC Bar)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34520179
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/452/179
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/452/179
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/452/179
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/452/179
Provenance
Creator Chiosi E.; Vallenari A.; Held E.V.; Rizzi L.; Moretti A.
Publisher CDS
Publication Year 2007
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