DARK MATTER SCALING RELATIONS AND THE ASSEMBLY EPOCH OF COMA EARLY-TYPE GALAXIES
Axisymmetric, orbit-based dynamical models are used to derive dark matter scaling relations for Coma early-type galaxies. From faint to bright galaxies, halo core radii and asymptotic circular velocities increase. Compared to spirals of the same brightness, the majority of Coma early-type galaxies -...
| المؤلفون الرئيسيون: | , , , , , , , |
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| التنسيق: | Journal article |
| اللغة: | English |
| منشور في: |
Institute of Physics Publishing
2009
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