Stellar secular parallaxes, derived from the absolute proper motions in the general catalog of the MEGA program

Details Stellar secular parallaxes, derived from the absolute proper motions in the general catalog of the MEGA program Stellar secular parallaxes, derived from the absolute proper motions in the general catalog of the MEGA program

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...24k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Sept.-Oct. 1989, p. 24-27. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Catalogs, Secular Variations, Stellar Motions, Stellar Parallax, Astrometry, Milky Way Galaxy, Stellar Magnitude

Scientific paper

The secular parallaxes of stars with magnitudes in the range B = 9-16 m
are determined using the absolute proper motions from the general
catalog of the Mega/AGK3 program. The weighted mean values of stellar
secular parallaxes based on the data of various authors are calculated
for high, intermediate, and low Galactic latitudes.

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