Revisiting the open cluster Lo 807

Details Revisiting the open cluster Lo 807 Revisiting the open cluster Lo 807

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ap%26ss.319..125w&link_type=abstract

Astrophysics and Space Science, Volume 319, Issue 2-4, pp. 125-129

Astronomy and Astrophysics

Astrophysics

1

Galaxy: Open Cluster, Membership, Astrometry, Photometry: Near-Infrared

Scientific paper

We have conducted an astrometric study of the open cluster Lo 807 using proper motion data from UCAC2 catalog. We applied the maximum likelihood method to determine cluster membership by using the proper motion data. The Padova isochrones lines with solar metallicity were fitted upon the Color Magnitude Diagram in near-infrared to derive physical parameters of the cluster. We do not detect significant variable reddening within the cluster. The present result is compared with our previous study.

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