RW Comae Berencies. I - Early photometry and UBV light curves

Details RW Comae Berencies. I - Early photometry and UBV light curves RW Comae Berencies. I - Early photometry and UBV light curves

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apjs...43..339m&link_type=abstract

Astrophysical Journal Supplement Series, vol. 43, June 1980, p. 339-364. Research supported by the University of Calgary and Na

Astronomy and Astrophysics

Astrophysics

16

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Ubv Spectra, Asymmetry, Infrared Photometry, Tables (Data)

Scientific paper

The analysis deals with the results of photometric observations of the eclipsing binary RW Com and with all published light curves of this object. The analysis reveals a variable asymmetric light curve and a variable period in all the cases studied. The system is found to be redder at all phases than is expected from early- to mid-G components, but there is a tendency for the bright maximum to be slightly bluer. The present work is seen to provide a basis for spectroscopic and infrared photometry studies and for analyses of system models, intrinsic properties of RC Com, and the origin of the asymmetry.

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