| Photometric solution for the eclipsing binary TT Aurigae (1982) | |||||||||||||
Abstract | |||||||||||||
| Photometric elements of TT Aur are derived from the UBV observations of the star during 1973-77. The system is found to be detached but quite close. Absolute dimensions are obtained on the basis of the spectroscopic element given by Joy & Sitterly (1931). It appears that the radial velocity amplitudes found by them might need upward revision by about 50 km/s. | |||||||||||||
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