Photoelectric Photometry and Further Discussions of V Cephei
Volume 17 number 2 (1988)
- Russell E. Milton
- David B. Williams
- Dorrit Hoffleit
Abstract
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.