Properties of the main-sequence eclipsing binary UZ Draconis
Makaleler > Tam Makale · 1989
Yazarlar: Claud H. Lacy, Omur Gulmen, Necdet Gudur, Cengiz Sezer
The Astronomical Journal, Uluslararası, 1989, cilt 97, ss 822-822
DOI: 10.1086/115028
Özet
The fundamental properties of the main-sequence binary, UZ Dra, are determined from observational data. Photoelectric radial-velocity measurements (Imbert, 1986), spectroscopic data obtained with solid-state array detectors, and B,V photoelectric light curves of the binary are examined. The properties of the stars in the binary are presented and compared with those of other F-type main-sequence binaries listed by Popper (1980).