BVIc photometry in Lynga 11

We have obtained CCD BVI_KC_ photometry down to V~21.5 for the open cluster Lynga 11 and its surrounding field. This previously unstudied object appears to be rich and highly absorbed. A cluster angular radius of 4.5+/-0.5, equivalent to (3.0+/-0.3)pc, is estimated from star counts in 100-pixel a side boxes distributed throughout the whole observed field. Our analysis suggests that Lynga 11 is moderately young and probably of solar metallicity.

Cone search capability for table J/other/NewA/11.262/table1 (CCD BVI data of stars in the field of Lynga 11)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/other/NewA/11.262
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/NewA/11.262
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/NewA/11.262
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/other/NewA/11.262
Provenance
Creator Piatti A.E.; Claria J.J.; Ahumada A.V.
Publisher CDS
Publication Year 2006
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy