Kinematics of the Outer Pseudorings and the Spiral Structure of the Galaxy

Details Kinematics of the Outer Pseudorings and the Spiral Structure of the Galaxy Kinematics of the Outer Pseudorings and the Spiral Structure of the Galaxy

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010vsgh.conf..137m&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

Models of the Galaxy with an outer ring of class R_1R_2' reproduce well the residual velocities of OB associations in the Perseus and Sagittarius regions. The kinematics of young stars in the Perseus region indicates the presence of an R_2 ring while the velocities in the Sagittarius region suggest the existence of an R_1 ring in the Galaxy.

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