Speaker
Tobias Fritz
(MPE)
Description
I will present recent results for the nuclear cluster of Milky Way. Thereby, I concentrate on the old stars which dominate the mass budget.
Firstly, I show a star density map of the cluster and use it to give a new estimate for its size. Secondly, I present an estimate for its mass from Jeans modeling using 23000 velocities. Finally, I relate these two properties with each other and with other nuclear clusters to conclude.
Author
Tobias Fritz
(MPE)