Mean parallaxes and the number of stars down to 23rd magnitude in the BVR system.

Details Mean parallaxes and the number of stars down to 23rd magnitude in the BVR system. Mean parallaxes and the number of stars down to 23rd magnitude in the BVR system.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996kpcb...12...28k&link_type=abstract

Kinematics Phys. Celest. Bodies, Vol. 12, No. 6, p. 28 - 37

Statistics

Stellar Statistics: Parallaxes, Stellar Statistics: Galaxy

Scientific paper

The author presents mean parallaxes and the number of stars down to 23rd magnitude in Johnson's BVR system, which corresponds to present-day observational material. The data were calculated on the basis of two integral equations of stellar statistics with the use of the model of the Galaxy which involves a disk with main-sequence stars and giants of population I, a thick disk, and a spheroid. The mean parallaxes are calculated for intervals of 10° and 45° on the Galactic latitude and longitude, respectively.

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