BVR Photometry of the Three RS CVn Binary Stars: V711 Tau, UX Ari and IM Peg

Details BVR Photometry of the Three RS CVn Binary Stars: V711 Tau, UX Ari and IM Peg BVR Photometry of the Three RS CVn Binary Stars: V711 Tau, UX Ari and IM Peg

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.235..337p&link_type=abstract

Astrophysics and Space Science, Volume 235, Issue 2, pp.337-341

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

Differential BVR photometric observations of the three RS CVn binary stars: V711 Tau, UX Ari and IM Peg obtained during the period November 26, 1994 February 24, 1995 using the 0.35 m reflector telescope equipped with photoelectric photometer are presented. Analysis of light curves shows significant changes in shape, amplitude as well as the phases of minimum light of all the three binaries. The amplitude of IM Peg, in particular, is found to have reached a larger value in the present epoch of observation than reported earlier.

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