Apsidal motion of the eccentric eclipsing binary GSC 4487-0347

Details Apsidal motion of the eccentric eclipsing binary GSC 4487-0347 Apsidal motion of the eccentric eclipsing binary GSC 4487-0347

Apr 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ibvs.6020....1k&link_type=abstract

Information Bulletin on Variable Stars, 6020, 1.

Computer Science

Ccd-Photometry, Spectrophotometry, Binaries:Eclipsing

Scientific paper

The eclipsing variable star GSC 4487-0347 is a recently discovered binary system. We carried out observations of the eclipsing binary using a CCD-array in 2009, 2011 at the Tien Shan Observatory. The B,V,R magnitudes were measured and the spectral range of components were estimated. The photometric elements were derived from the light curve. We found the apsidal period is U=160+-6 years.

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