The flattening and the orbital structure of early-type galaxies and collisionless N-body binary disc mergers
We use oblate axisymmetric dynamical models including dark haloes to determine the orbital structure of intermediate mass to massive early-type galaxies in the Coma galaxy cluster. We find a large variety of orbital compositions. Averaged over all sample galaxies the unordered stellar kinetic energy...
Váldodahkkit: | Thomas, J, Jesseit, R, Saglia, R, Bender, R, Burkert, A, Corsini, E, Gebhardt, K, Magorrian, J, Naab, T, Thomas, D, Wegner, G |
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Materiálatiipa: | Journal article |
Giella: | English |
Almmustuhtton: |
2009
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Geahča maid
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