BV photometry of 6 SMC stellar clusters

DOI

Stellar clusters in the Small Magellanic Cloud (SMC) are useful probes to study the chemical and dynamical evolution of this neighbouring dwarf galaxy, enabling inspection of a large period covering over 10Gyr. The main goals of this work are the derivation of age, metallicity, distance modulus, reddening, core radius and central density profile for six sample clusters, in order to place them in the context of the Small Cloud evolution. The studied clusters are: AM 3, HW 1, HW 34, HW 40, Lindsay 2, and Lindsay 3, where HW 1, HW 34, and Lindsay 2 are studied for the first time. Optical Colour-Magnitude Diagrams (V, B-V CMDs) and radial density profiles were built from images obtained with the 4.1m SOAR telescope, reaching V~23. The determination of structural parameters were carried out applying King profile fitting. The other parameters were derived in a self-consistent way by means of isochrone fitting, which uses the likelihood statistics to identify the synthetic CMDs that best reproduce the observed ones. Membership probabilities were determined comparing the cluster and control field CMDs. Completeness and photometric uncertainties were obtained performing artificial star tests. The results confirm that these clusters (except HW 34, identified as a field fluctuation) are intermediate-age clusters, with ages between 1.2Gyr (Lindsay 3) and ~5.0Gyr (HW 1). In particular HW 1, Lindsay 2, and Lindsay 3 are located in a region that we called West Halo, where studies on ages and metallicity gradients are still lacking. Moreover Lindsay 2 was identified as a moderately metal-poor cluster with [Fe/H]=-1.4+/-0.2dex, lower than expected from the age-metallicity relation by Pagel & Tautvaisiene (1998MNRAS.299..535P). We also found distances varying from ~53 to 66kpc, compatible with the large depth of the SMC.

Cone search capability for table J/A+A/561/A106/table1 (Log of observations)

Cone search capability for table J/A+A/561/A106/am3 (Star coordinates, magnitudes, completeness and membership probability for AM3)

Cone search capability for table J/A+A/561/A106/hw1 (Star coordinates, magnitudes, completeness and membership probability for HW1)

Cone search capability for table J/A+A/561/A106/hw34 (Star coordinates, magnitudes, completeness and membership probability for HW34)

Cone search capability for table J/A+A/561/A106/hw40 (Star coordinates, magnitudes, completeness and membership probability for HW40)

Cone search capability for table J/A+A/561/A106/l2 (Star coordinates, magnitudes, completeness and membership probability for Lindsay2)

Cone search capability for table J/A+A/561/A106/l3 (Star coordinates, magnitudes, completeness and membership probability for Lindsay3)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35610106
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/561/A106
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/561/A106
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/561/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/561/A106
Provenance
Creator Dias B.; Kerber L.; Barbuy B.; Santiago B.; Ortolani S.; Balbinot E.
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy