Eric Emsellem edited section_Milky_Way_simulation_Emsellem__.tex  about 9 years ago

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\url{http://irfu.cea.fr/Pisp/florent.renaud/mw_large.php}  See ref paper = Renaud et al. 2013, MNRAS 436 1836  and Emsellem et al. 2015, MNRAS 446, 2446  Relative Milky Way BH and nuclear cluster mass is an order of magnitude less than in simulation, BH / CMZ (MW) $\sim0.1$ BH/CMZ(sim)