Kinematics of a system of globular clusters and the distance to the center of the Galaxy

Details Kinematics of a system of globular clusters and the distance to the center of the Galaxy Kinematics of a system of globular clusters and the distance to the center of the Galaxy

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990velen......108n&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), Oct. 1990, p. 108, 109. In Russian.

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Galactic Structure, Globular Clusters, Galactic Clusters, Radial Velocity, Rangefinding

Scientific paper

The distance to the center of the Galaxy is estimated from an analysis
of the radial velocities of Galactic globular clusters using the maximum
correspondence method. The kinematic parameters of a system of globular
clusters obtained for R0 = 7 kpc are presented.

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