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A formal approach to stellar positions in solar barycentric coordinates
Published online by Cambridge University Press: 04 August 2017
Abstract
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In astrometry, construction of stellar catalogues favors solar barycentric coordinates. Classically, they are calculated by linearly removing stellar aberration and annual parallaxes from measured quantities yielded by Earth-bound instruments. A global approach is proposed to account for those two effects from a more general relativistic point of view. Implications for VLBI measurements and HIPPARCOS measurements of stellar positions are discussed.
- Type
- Reference Frames and Astrometry
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- Copyright
- Copyright © Reidel 1986
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