Visual and Photographic Orbital Mean Light Curves for the Recurrent Nova T Coronae Borealis

Details Visual and Photographic Orbital Mean Light Curves for the Recurrent Nova T Coronae Borealis Visual and Photographic Orbital Mean Light Curves for the Recurrent Nova T Coronae Borealis

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985javso..14....8p&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 14, no. 1, p. 8-11

Physics

6

Scientific paper

Mean orbital light curves of T CrB at quiescence are derived from previously unreduced 1872-1904 visual estimates of T. W. Backhouse and partly concurrent Harvard photographic observations. They agree in showing ellipsoidal minima with different depths, an irregularity near where hot-spot influence might be expected, and primary minima not midway between secondary minima. A marginally refined orbital period of 227.52 +/- 0.05 days is suggested.

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