Corrections to the lunisolar precession and the motion of the equinox from proper motions of Cepheids |
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Authors: | A. M. Sinzi |
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Affiliation: | (1) Astronomical Division, Hydrographic Department, Tokyo, Japan |
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Abstract: | Corrections to Newcomb's lunisolar precession and to motion of the equinox are evaluated from proper motions of 77 Cepheids, employing recently determined values of their distances. Results are diverse, depending on the weighting method. If the effect of the cosmic dispersion is neglected and 0 is imposed to be 25 km/s/kpc, then p1=1 .1±0 .2 and  + e = 1 .0 ± 0 .1 per century in the FK4 system.Presented at IAU Colloquium No. 9, The IAU System of Astronomical Constants , Heidelberg, Germany, August 12–14, 1970. |
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