Infrared Photometry of Uv-Piscium
Abstract
The eclipsing binary system UV Psc was observed in the near-infrared (JHK), and a wave-like distortions have been observed similar to those in the visible. The out-of-eclipse observations have shown real large amount of scatter. This cannot be attributed to the existence of spots on one of the components, which can explain the wave-like distorition of the light curves, but probably to the intrinsic variability of one of them.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- July 1987
- DOI:
- 10.1007/BF00641569
- Bibcode:
- 1987Ap&SS.135..335A
- Keywords:
-
- Eclipsing Binary Stars;
- Infrared Photometry;
- Light Curve;
- Near Infrared Radiation;
- Magnitude;
- Photographic Plates;
- Astrophysics