Determination of parameters of W UMa system. V - V757 Cen, ER Cep, AH CNC

Details Determination of parameters of W UMa system. V - V757 Cen, ER Cep, AH CNC Determination of parameters of W UMa system. V - V757 Cen, ER Cep, AH CNC

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26as...58..405m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 58, Nov. 1984, p. 405-410. Research supported by the Consigl

Astronomy and Astrophysics

Astrophysics

8

Eclipsing Binary Stars, Light Curve, Astronomical Models, Astronomical Spectroscopy, Electrophotometry

Scientific paper

From photoelectric and spectroscopic data available in the literature, the elements of three W Ursae Majoris systems have been determined by means of the Roche-model-based method of Wilson and Devinney (1971). According to the presented solutions, the three systems (V757 Cen, ER Cep, AH Cnc) are all of W-type, that is, primary minima are caused by occultation of the smaller (and less massive) component.

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