Polarimetry of stars in NGC 5617 Virtual Observatory Resource

Authors

1. Orsatti A.M.
2. Feinstein C.
3. Vergne M.M.
4. Martinez R.E.
5. Vega E.I.

Published by

CDS

Abstract

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.

Keywords

1. Open star clusters
2. Polarimetry

Bibliographic source Bibcode

2010A&A...513A..75O

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doi:10.26093/cds/vizier.35130075

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