Photoelectric Photometry and Further Discussions of V Cephei

Details Photoelectric Photometry and Further Discussions of V Cephei Photoelectric Photometry and Further Discussions of V Cephei

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988javso..17..137m&link_type=abstract

The Journal of the American Association of Variable Star Observers. vol. 17, no. 1, p. 137-140

Computer Science

2

V Cephei

Scientific paper

Photoelectric observations on 34 nights during a 428-day interval in
1986-87 indicate that V Cep and the comparision star HR 158 (NSV-235)
were constant within +-0.02 magnitude. An explanation for the
variability found by some visual observers is discussed.

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