The Determination of the Equator-Point for Observing Star Declinations

The deolinations of the stars are by definition reckoned from the celestial equator. However this great circle is not marked on the sky; therefore, instead of dejclinations, the polar distances of the stars are measured, as the position of the pole can be found by observing a star in upper and lower...

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Bibliographic Details
Published in:International Astronomical Union Colloquium
Main Author: Mikhailov, A. A.
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 1975
Subjects:
Online Access:http://dx.doi.org/10.1017/s0252921100051125