Infrared photometry of UV PISCIUM

Details Infrared photometry of UV PISCIUM Infrared photometry of UV PISCIUM

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.135..335a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 135, no. 2, July 1987, p. 335-345.

Astronomy and Astrophysics

Astrophysics

4

Eclipsing Binary Stars, Infrared Photometry, Light Curve, Near Infrared Radiation, Magnitude, Photographic Plates

Scientific paper

The eclipsing binary system UV Psc was observed in the near-infrared (JHK), and wave-like distortions have been observed similar to those in the visible. The out-of-eclipse observations have shown a very large amount of scatter. This cannot be attributed to the existence of spots on one of the components, which can explain the wave-like distortion of the light curves, but probably to the intrinsic variability of one of them.

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