Radial velocities for contact binary systems. III - V566 Ophiuchi

Details Radial velocities for contact binary systems. III - V566 Ophiuchi Radial velocities for contact binary systems. III - V566 Ophiuchi

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204..817m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, Aug. 1983, p. 817-820.

Astronomy and Astrophysics

Astronomy

25

Binary Stars, Radial Velocity, Stellar Spectra, Data Reduction, Mass Ratios, Spectrographs

Scientific paper

Radial velocity observations obtained using a digital reduction
technique are presented for the W Ursae Majoris system V566 Oph. The
derived spectroscopic mass ratio is found to be in good agreement with
the photometric value determined using light curve synthesis techniques.

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