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Eric Emsellem edited section_Milky_Way_simulation_Emsellem__.tex
about 9 years ago
Commit id: 5a08fab7455c638f5f08de0937a2dbcd29b55e30
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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)