Photometric behaviour of the interacting binary V 1914 Cygni

Details Photometric behaviour of the interacting binary V 1914 Cygni Photometric behaviour of the interacting binary V 1914 Cygni

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...232..381s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 232, no. 2, June 1990, p. 381, 382.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Photometry, B Stars, Eclipsing Binary Stars, F Stars, Variable Stars, Accretion Disks, Cygnus Constellation, H Alpha Line, Light Curve, Stellar Color, Stellar Orbits, Ubv Spectra

Scientific paper

New photoelectric observations of the interacting binary HD 207739 = V
1914 Cyg are presented. An orbital period of 141.25 d is determined. The
light and color curves and their phase relation to the radial velocity
changes are in agreement with the accretion disk model of this eclipsing
binary star suggested by Parsons et al. (1988).

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