New photoelectric observations and elements of the eclipsing W UMa-type system V839 OPH

Details New photoelectric observations and elements of the eclipsing W UMa-type system V839 OPH New photoelectric observations and elements of the eclipsing W UMa-type system V839 OPH

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.153..143n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 153, no. 1, March 1989, p. 143-152.

Physics

Optics

8

Eclipsing Binary Stars, Stellar Spectrophotometry, Cassegrain Optics, Light Curve, Mass Transfer, Stellar Magnitude

Scientific paper

The W UMa-type system V839 Oph was observed photoelectrically in two wavebands (B and V) during 1985 at the Kryonerion Astronomical Station of the National Observatory of Greece. The light curves of the system are analyzed using the frequency-domain techniques and new geometric and photometric elements are given. The light variations of the system are also discussed.

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