The Secondary Period of TU Comae Berenices

Details The Secondary Period of TU Comae Berenices The Secondary Period of TU Comae Berenices

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976javso...4..103m&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 4, no. 1, p. 103-104

Physics

Variables, Rr Lyrae Stars, Tu Com

Scientific paper

Photographic observations between 1928 and 1975 have been analyzed to
derive a secular decrease of period. A secondary period of about 40
days in the times of maxima is reported.

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