Polarimetry of stars in NGC 5617

DOI

We present polarimetric observations in the UBVRI bands of 72 stars located in the direction of the medium age open cluster NGC 5617. Our intention is to use polarimetry as a tool in membership identification, by building on previous investigations intended mainly to determine the cluster's general characteristics rather than provide membership suitable for studies such as stellar content and metallicity, as well as study the characteristics of the dust lying between the Sun and the cluster.

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Identifier
DOI http://doi.org/10.26093/cds/vizier.35130075
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/513/A75
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/513/A75
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/513/A75
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/513/A75
Provenance
Creator Orsatti A.M.; Feinstein C.; Vergne M.M.; Martinez R.E.; Vega E.I.
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; Exoplanet Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy