Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.253..710v&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 253, Dec. 15, 1991, p. 710-726.
Astronomy and Astrophysics
Astronomy
244
Elliptical Galaxies, Mass To Light Ratios, Velocity Distribution, Anisotropy, Astronomical Models, Astronomical Photometry, Dynamic Models, Galactic Structure
Scientific paper
The kinematics are predicted for 37 bright elliptical galaxies for which axisymmetric dynamical models are developed and for which both photometrical and major- and minor-axis kinematical data exist. Assumptions are made including a velocity ellipsoid and a constant mass-to-light ratio, and the model predictions are analyzed critically. Because the models predict too much motion on the major axis it is proposed that the elliptical galaxies have a velocity ellipsoid that has not previously been shown. The results support the validity of N-body simulations of dissipationless collapse, and mass-to-light ratios from the models are corrected for rotation and radial anisotropy. Because the observed galaxy velocities systematically exceed the model predictions, it is concluded that axisymmetric constant mass-to-light ratios are untenable. The conclusions suggest the presence of dark halos in the galaxies or the need for exploring triaxial models for the mass-to-light ratios.
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