Photometric Study Of W Uma Type Binary In The Old Cluster Ngc 6791

Details Photometric Study Of W Uma Type Binary In The Old Cluster Ngc 6791 Photometric Study Of W Uma Type Binary In The Old Cluster Ngc 6791

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.299..109r&link_type=abstract

Astrophysics and Space Science, Volume 299, Issue 2, pp.109-116

Astronomy and Astrophysics

Astrophysics

7

Binaries, Close-Binaries, Eclipsing-Stars, Individual (W Uma)-Stars, Late Type-Stars

Scientific paper

Study of eclipsing binaries in an open cluster offer information
regarding the age of the cluster in addition to the component stars. In
this paper we present the analysis of a W UMa system discovered in the
open cluster NGC 6791 using the Wilson Devinney (W D) method.

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