Astrometric Study of Lo 1339

Details Astrometric Study of Lo 1339 Astrometric Study of Lo 1339

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1283..327w&link_type=abstract

MATHEMATICS AND ASTRONOMY: A JOINT LONG JOURNEY: Proceedings of the International Conference. AIP Conference Proceedings, Volum

Computer Science

Databases

Clusters Of Galaxies, Astronomical Catalogues, Galaxy, Photometry, Galaxy Clusters, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Kinematics, Dynamics, And Rotation, Photometric, Polarimetric, And Spectroscopic Instrumentation

Scientific paper

We presented a preliminary result of astrometric study of galactic cluster Lo 1339 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, where we obtained the age of cluster log t = 8.4+/-0.2, the distance of 1284+/-140 pc, and the absorption AJ = 0.26+/-0.13 mag with cluster diameter of 4.9+/-0.5 pc.

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