1992 UBV observations of UV PISCIUM and light curve analysis

Details 1992 UBV observations of UV PISCIUM and light curve analysis 1992 UBV observations of UV PISCIUM and light curve analysis

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.219...35j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 219, no. 1, p. 35-47

Astronomy and Astrophysics

Astronomy

4

Eclipsing Binary Stars, Light Curve, Photosphere, Starspots, Ultraviolet Astronomy, Ultraviolet Photometry, Eclipses, Stellar Occultation, Stellar Spectrophotometry, Tables (Data)

Scientific paper

In 1992 UBV photometry of short period binary system UV PSc were presented. The results obtained from the analysis of U, B and V light curves represent 'transit' solutions. The light fluctuations of out-side eclipses have been interpreted in terms of cool star-spots on the photosphere of the primary component. Its parameters have been determined.

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