Fragmentation Instability of Molecular Clouds: Numerical Simulations

Abstract

We simulate fragmentation and gravitational collapse of cold, magnetized molecular clouds. We explore the nonlinear development of an instability mediated by ambipolar diffusion, in which the collapse rate is intermediate to fast gravitational collapse and slow quasistatic collapse. Initially uniform stable clouds fragment into elongated clumps with masses largely determined by the cloud temperature, but substantially larger than the thermal Jeans mass. The clumps are asymmetric, with significant rotation and vorticity, and lose magnetic flux as they collapse. The clump shapes, intermediate collapse rates, and infall profiles may help explain observations not easily fit by contemporary slow or rapid collapse models.

25pp, 20 small eps figures, in press ApJ, April 1, 2000

References in corpus (2)

• Physical Conditions in Regions of Star Formation
• Consistency of Ambipolar Diffusion Models with Infall in the L1544 Protostellar Core

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