Simple photometric observations of BR Canum Venaticorum (a troublesome comparison star)

Details Simple photometric observations of BR Canum Venaticorum (a troublesome comparison star) Simple photometric observations of BR Canum Venaticorum (a troublesome comparison star)

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jbaa..109..151w&link_type=abstract

Journal of the British Astronomical Association, vol.109, no.3, p.151-154

Astronomy and Astrophysics

Astronomy

Scientific paper

During the last four years an Optec SSP3 photometer has been used to obtain lightcurves for various suspected and confirmed variable stars. Upon analysis the semi-regular variable BR CVn (formerly a comparison star for V CVn) showed clear periods of 712 and 71 days, both periods having average peak-to-peak amplitudes of less than 0.3 magnitude. The total observed range using a V-band filter has been 6.47-7.17.

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