The survival of substructure in clumpy clusters

Details The survival of substructure in clumpy clusters The survival of substructure in clumpy clusters

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..385g&link_type=abstract

In: Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 J

Astronomy and Astrophysics

Astronomy

Dense Stellar Systems

Scientific paper

Initially fractal star clusters undergo a dramatic phase of dynamical evolution. Significant amount of substructure can remain in the clusters especially if the initial velocity field is correlated with the density structures. As observations show that many star clusters are born clumpy simulations with smooth initial conditions may be missing an important phase of cluster evolution.

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