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...
المؤلفون الرئيسيون: | 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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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
2009
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مواد مشابهة
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Specific angular momentum of disc merger remnants and the lambda(R)-parameter
حسب: Jesseit, R, وآخرون
منشور في: (2009) -
Dynamical modelling of luminous and dark matter in 17 Coma early-type galaxies
حسب: Thomas, J, وآخرون
منشور في: (2007) -
DARK MATTER SCALING RELATIONS AND THE ASSEMBLY EPOCH OF COMA EARLY-TYPE GALAXIES
حسب: Thomas, J, وآخرون
منشور في: (2009) -
Regularized orbit models unveiling the stellar structure and dark matter halo of the Coma elliptical NGC 4807
حسب: Thomas, J, وآخرون
منشور في: (2005) -
Dynamical masses of early-type galaxies: a comparison to lensing results and implications for the stellar initial mass function and the distribution of dark matter
حسب: Thomas, J, وآخرون
منشور في: (2011)