The determination of solar apex from high proper motion stars

Details The determination of solar apex from high proper motion stars The determination of solar apex from high proper motion stars

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005kfnt...21..317i&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 21, no. 4, p. 317-320

Astronomy and Astrophysics

Astrophysics

Scientific paper

Position of solar apex was determined using high proper motion stars
(μ ≥ 0.1l''/yr) of various spectral type from the compiled
list-catalogue of astrometrical and astrophysical data, which was
created in the Main Astronomical Observatory of National Academy of
Science of Ukraine.

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