On the Period of RR
Maria Mitchell Observatory,
Nantucket, MA 02554
Observations of the RR
Lyrae star, RR Canum Venaticorum, from 1932 to 1980 are satisfied by a constant
basic pulsation period on which are superimposed fluctuations due to changes in
the shape and amplitude of the light curve.
Link to ADS abstract, article and citation information
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