UBV observations of the eclipsing binary FW Monocerotis

Details UBV observations of the eclipsing binary FW Monocerotis UBV observations of the eclipsing binary FW Monocerotis

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.209...51s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 209, no. 1, p. 51-63

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Stellar Color, Stellar Magnitude, Stellar Systems, Ubv Spectra, Astronomical Photometry, Electrophotometers, Light Curve, Stellar Radiation

Scientific paper

Photoelectric observations of FW Monocerotis in U, B, and V filters have
been discussed. The depths of the primary minimum in UBV colors are 2.63
magnitudes, 2.17 magnitudes, and 1.76 magnitudes, respectively. No
variation in the period has been found and its revised value is
3.8735868 days.

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