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 -...

詳細記述

書誌詳細
主要な著者: Thomas, J, Saglia, R, Bender, R, Thomas, D, Gebhardt, K, Magorrian, J, Corsini, E, Wegner, G
フォーマット: Journal article
言語:English
出版事項: Institute of Physics Publishing 2009

類似資料