The Structural Approach to the Subsystems of the Galaxy

Details The Structural Approach to the Subsystems of the Galaxy The Structural Approach to the Subsystems of the Galaxy

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010vsgh.conf..165s&link_type=abstract

Variable Stars, the Galactic halo and Galaxy Formation, Proceedings of an international conference held in Zvenigorod, Russia, 1

Astronomy and Astrophysics

Astronomy

Scientific paper

We assume that the subsystems of the Galaxy (populations) consist of inclined discrete structures (belts) and depend on their inclination angle i (from 0 to 90°). The subsystem boundaries are skirting these belts. The survival of the inclined belts in the differentially rotating Galaxy may depend both on the age and on the peculiarities in kinematics. We also consider differences between mean radial velocities (or proper motions) between belts symmetrical with respect to the Milky Way.

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