Das Geschwindigkeitsellipsoid der H II-Regionen in M33

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The peculiar radial velocities of Hii regions in M33 varies with
position angle in a manner that can be explained by an ellipsoidal
distribution with minor axis in the direction of rotation. The amplitude
of the variations, however, is too great as compared with theory or
experience in the galaxy.

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