Uy-Phoenicis - Rr-Lyrae Variable not Dwarf Nova
Abstract
Photometric and spectroscopic observations of UY Phe, previously classified as a dwarf nova, show it to be a typea RR Lyr halo variable with a period of 0.5118 day.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- July 1986
- DOI:
- 10.1007/BF00649760
- Bibcode:
- 1986Ap&SS.124..199W
- Keywords:
-
- Brightness;
- Cepheid Variables;
- Dwarf Novae;
- Variable Stars;
- A Stars;
- Astronomical Photometry;
- Astronomical Spectroscopy;
- Cataclysmic Variables;
- Light Curve;
- Astrophysics