Stability of Galactic Gaseous Disks and the Formation of Massive Clusters
Description:
We study gravitational instabilities in disks, with special attention to the most massive clumps that form because they are expected to be the progenitors of globular-type clusters. The maximum unstable mass is set by rotation and depends only on the surface density and orbital frequency of the disk. We propose that the formation of massive clusters is related to this largest scale in galaxies not stabilized by rotation. Using data from the literature, we predict that globular-like clusters can…
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Date:
August 21, 2008
Creator:
Escala, Andres & Larson, Richard B.
Partner:
UNT Libraries Government Documents Department