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 \cite{Renaud_2013}  and Emsellem et al. 2015, MNRAS 446, 2446 \cite{Emsellem_2014}  Relative Milky Way BH and nuclear cluster mass is may be  an order of magnitude less than in simulation, BH / CMZ (MW) $\sim0.1$ BH/CMZ(sim) but to be checked.