Kinematics of the Supercomplex of open star clusters

Details Kinematics of the Supercomplex of open star clusters Kinematics of the Supercomplex of open star clusters

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6....3n&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Sept.-Oct. 1990, p. 3-7. In Russian.

Statistics

Computation

Molecular Clouds, Open Clusters, Star Clusters, Angular Velocity, Astronomical Catalogs, Computational Astrophysics, Kinematics

Scientific paper

The kinematics of the 'Supercomplex' is studied using the
Ogorodnikov-Milne method applied to space velocities of clusters
relative to the quasi-circular velocity. The rotation of the
Supercomplex with an angular velocity of 10 + or - 2 km/s kpc is
confirmed, and the contraction of the Supercomplex is observed.

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