A 'symmetrical' kinematical model for elliptical galaxies - Application to the edge on bulge of M31

Details A 'symmetrical' kinematical model for elliptical galaxies - Application to the edge on bulge of M31 A 'symmetrical' kinematical model for elliptical galaxies - Application to the edge on bulge of M31

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...102..175m&link_type=abstract

Astronomy and Astrophysics, vol. 102, no. 2, Oct. 1981, p. 175-177.

Astronomy and Astrophysics

Astrophysics

1

Andromeda Galaxy, Astronomical Models, Elliptical Galaxies, Galactic Bulge, Galactic Structure, Kinematics, Angular Momentum, Dynamic Models, Radial Velocity, Stellar Luminosity, Stellar Motions, Symmetry

Scientific paper

We have derived a kinematical model for elliptical galaxies, under the assumptions of cylindrical symmetry of the residual velocities and the absence of third order velocity asymmetries. It is shown to be in correct agreement with known experimental data on the bulge of M31, and to give a M/L ratio very similar to that computed for very different assumptions.

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