Radial velocities for contact binary systems – III. V566 Ophiuchi

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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Published in:Monthly notices of the Royal Astronomical Society 1983-10, Vol.204 (3), p.817-820
Main Author: McLean, B. J.
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Language:English
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description 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.
doi_str_mv 10.1093/mnras/204.3.817
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title Radial velocities for contact binary systems – III. V566 Ophiuchi
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