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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 |
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| Main Author: | |
| Format: | Article |
| Language: | English |
| Citations: | Items that cite this one |
| Online Access: | Get full text |
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| Summary: | 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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| ISSN: | 0035-8711 1365-2966 |
| DOI: | 10.1093/mnras/204.3.817 |