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Protostellar Collapse Induced by Compression
Authors:Hennebelle Patrick  Belloche Arnaud  Whitworth Anthony  André Philippe
Institution:1. Laboratoire de radioastronomie millimétrique, UMR, Paris, France
2. Department of Physics and Astronomy, Cardiff University, Wales, UK
3. CEA, DSM, DAPNIA, Service d'Astrophysique, C.E. Saclay, Gif-sur-Yvette Cedex, France
Abstract:We present numerical simulations of the evolution of low-mass, isothermal, molecular cores which are subjected to an increase in external pressure. If the external pressure increases very slowly, the core approaches instability quite quasi-statically. However, for faster compressions, a compression wave is driven into the core (Hennebelle, P., Whitworth, A., Gladwin, P. and André, P.: 2003a MNRAS 340, 870). Quantitative comparisons with observational velocity and density profiles are presented. The consequences of this compression for the fragmentation of the cloud is investigated and discussed.
Keywords:
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