A photoelectric study of the W UMa-system U Pegasi

Details A photoelectric study of the W UMa-system U Pegasi A photoelectric study of the W UMa-system U Pegasi

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.121...61l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 121, no. 1, April 1986, p. 61-81.

Astronomy and Astrophysics

Astrophysics

11

Astronomical Photometry, Eclipsing Binary Stars, Electrophotometry, Light Curve, Optimization, Periodic Variations

Scientific paper

The W UMa-system U Pegasi was observed photoelectrically in two
wavebands (B and V) in 1984. The light curves of this system are
analysed using Kopal's frequency-domain technique and the optimisation
method. New geometrical and physical elements have been determined and
the period-variations discussed.

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