A. O. Gromov, I. I. Nikiforov, L. P. Ossipkov
Published 2015-08-21Version 1
An earlier derived quasi-isothermal St\"ackel's model of mass distribution in stellar systems and the corresponding formula for space density are applied to our Galaxy. The model rotation curve is fitted to HI kinematical data. The structural and scale parameters of the model are estimated and the corresponding density contours for our Galaxy are presented.
Comments: 7 pages, 3 figures. Accepted for publication in Baltic Astronomy (BA)
Journal: Baltic Astronomy. 24: No. 2, 150-156, 2015
Rotation Curve and Mass Distribution in the Galaxy from the Velocities of Objects at Distances up to 200 kpc
The link between mass distribution and starbursts in dwarf galaxies
Mass Distribution in the Central Few Parsecs of Our Galaxy
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