this is for holding javascript data
Eric Emsellem edited section_Milky_Way_simulation_Emsellem__.tex
about 9 years ago
Commit id: ac3c3e41b44f6229a527aa7bd2b0c902f19fc479
deletions | additions
diff --git a/section_Milky_Way_simulation_Emsellem__.tex b/section_Milky_Way_simulation_Emsellem__.tex
index faf9e3e..a8c4368 100644
--- a/section_Milky_Way_simulation_Emsellem__.tex
+++ b/section_Milky_Way_simulation_Emsellem__.tex
...
See ref paper = \cite{Renaud_2013} and \cite{Emsellem_2014}
Relative Milky Way BH and nuclear cluster mass may be an order of magnitude less than in simulation, BH / CMZ (MW) $\sim0.1$ BH/CMZ(sim) but to be checked.
Clearly the mass ratio, extent, etc will decide on the fate, and cycle (if cycle there is).