Photoelectric photometry of HD 5303

Details Photoelectric photometry of HD 5303 Photoelectric photometry of HD 5303

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.202..427c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 202, Feb. 1983, p. 427-435.

Astronomy and Astrophysics

Astronomy

21

Binary Stars, Electrophotometry, Stellar Spectrophotometry, Variable Stars, Eclipsing Binary Stars, Electrophotometers, Light Curve, Radial Velocity, Reflectance

Scientific paper

The Bamberg variable HD 5303 is found to be a close binary system with
period 2.79786 ± 0.00002 day. The light curve has a photometric
wave of range 0.057 mag outside eclipse consistent with a dark spot or
spots on the cooler star. The eclipse elements together with the (B-V)
measurements show the system to be of type G0 + K4 IV.

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