A re-analysis of the light period of VZ CANCRI

Details A re-analysis of the light period of VZ CANCRI A re-analysis of the light period of VZ CANCRI

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acasn..32..397c&link_type=abstract

(Acta Astronomica Sinica, vol. 32, no. 4, 1991, p. 397-401) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 16, no. 2,

Astronomy and Astrophysics

Astrophysics

4

Cepheid Variables, Dwarf Stars, Light Curve, Astronomical Photometry, Periodic Variations, Stellar Oscillations, Synchronism

Scientific paper

Nine times of light maximum of VZ Cnc observed in 1985 and 1990 are
presented. Utilizing the data of 144 light maximum times obtained over
40 years, a reanalysis of the light period is performed. Using the known
method of calculating beat period and phase, a difference of about 0.2
between the calculated phase and the published phase is determined.

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