Will a nuclear stellar disk form in the galaxy Henize 2-10?
  We present results of a set of $N$-body simulations to model the future
evolution of the 11 young massive clusters hosted in the central region of the
dwarf starburst galaxy Henize 2-10, which contains at its center a massive
black hole with a mass $M_{\rm BH} \simeq 2\times 10^6$ M$_\odot$. Nuclear star
clusters are present in a great quantity of galaxies of mass similar to Henize
2-10. Our results \citep{ASCD15} show that the orbital decay and merging of the
Henize 2-10 clusters will likely lead to the formation of a nuclear star
cluster with mass $M_{\rm NSC} \simeq 4-6 \times 10^6$ M$_\odot$ and effective
radius $r_{\rm NSC} \simeq 4.1$ pc. Additionally, we found that this mechanism
can lead to the formation of disky structures with global properties similar to
those of nuclear stellar disks, which reside in many "middle-weight" galaxies.
This work confirms and enlarge recent results \citep{ASCDS15} that indicate how
nuclear star clusters and super massive black holes are only partially
correlated, since the formation process of nuclear star clusters is poorly
affected by a black hole of the size of that in Henize 2-10. A new result is
that nuclear star clusters and nuclear stellar disks may share the same
formation path.
