Photometric study of W UMa type binaries in the intermediate open cluster NGC 7789

Details Photometric study of W UMa type binaries in the intermediate open cluster NGC 7789 Photometric study of W UMa type binaries in the intermediate open cluster NGC 7789

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010raa....10..159s&link_type=abstract

Research in Astronomy and Astrophysics, Volume 10, Issue 2, pp. 159-165 (2010).

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

The light curve solutions of two W UMa binary systems in the intermediate open cluster NGC 7789 are presented in this paper. These variables were observed using the 2 m telescope of the IUCAA-Girawali Observatory. The V passband photometric solutions of the two W UMa binaries were obtained using the latest version of the W-D program. The result shows that both systems are H-subtype W UMa binaries with high mass ratios.

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