Clusters and associations in SMC and LMC

DOI

We investigate the degree of spatial correlation among extended structures in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). To this purpose, we work with subsamples characterized by different properties such as age and size, taken from the updated catalogue of Bica et al. (2008, Cat. J/MNRAS/389/678), or gathered in the present work. The structures are classified as star clusters or non-clusters (basically, nebular complexes and their stellar associations).

Cone search capability for table J/MNRAS/403/996/table2 (Old SMC and LMC clusters from CMDs, COLours and PLAte inspections)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74030996
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/403/996
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/403/996
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/403/996
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/403/996
Provenance
Creator Bonatto C.; Bica E.
Publisher CDS
Publication Year 2010
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; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy