Figure 3.
N-body results of M⋆ (top), rh (middle), and MBH (bottom) of isolated star clusters with different initial densities with BH kicks applied (dashed lines). Best-fitting clusterBH models are shown as full lines.

N-body results of M⋆ (top), rh (middle), and MBH (bottom) of isolated star clusters with different initial densities with BH kicks applied (dashed lines). Best-fitting clusterBH models are shown as full lines.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close