Authors: S D Wiramihardja M I Arifyanto Y Sugianto
Publish Date: 2009/01/08
Volume: 319, Issue: 2-4, Pages: 125-129
Abstract
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 nearinfrared 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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