Rotation, Statistical Dynamics and Kinematics of Globular Clusters

Details Rotation, Statistical Dynamics and Kinematics of Globular Clusters Rotation, Statistical Dynamics and Kinematics of Globular Clusters

2000-07-10

arxiv.org/abs/astro-ph/0007116v1

Astronomy and Astrophysics

Astrophysics

12 pages, Latex, 2 EPS Figures

Scientific paper

Evolution with mass segregation and the evolution of the rotation of cores are both discussed for self-similar core collapse. Evolution with angular velocity proportional to the square root of the density is predicted. On the Dynamical Main Sequence of globular clusters the energy emission from binaries balances the energy expended in expanding the halo. Newton's exactly solved N-body problem is then given, along with recent generalisations, all of which have no violent relaxation, but a new type of statistical equilibrium is discussed. Finally, we set the creation of streams in the Galaxy's halo in the historical context of their discovery.

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