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The Formation of Star Clusters I: 3D Simulations...
Preprint

The Formation of Star Clusters I: 3D Simulations of Hydrodynamic Turbulence

Abstract

We present the results of a series of numerical simulations of compressible, self-gravitating hydrodynamic turbulence of cluster-forming clumps in molecular

Authors

Tilley DA; Pudritz RE

Publication date

June 4, 2004

DOI

10.48550/arxiv.astro-ph/0406122

Preprint server

arXiv