BV photometry of NGC 1866

DOI

We present a new deep (down to V~24) photometry of a wide region (~6'x6') around the Large Magellanic Cloud globular cluster NGC 1866. Our sample is much larger (by more than a factor of 3) than any previous photometry and with a main sequence (MS) that may be considered complete, down to at least 3 mag below the brightest MS star; such an occurrence allows a meaningful and robust comparison with various theoretical scenarios produced by means of models computed with the evolutionary code FRANEC.

Cone search capability for table J/AJ/118/2839/stars (Photometry of stars in cluster and field frames)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51182839
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/118/2839
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/118/2839
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/118/2839
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/118/2839
Provenance
Creator Testa V.; Ferraro F.R.; Chieffi A.; Straniero O.; Limongi M.; Fusi Pecci F.
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy