Fragmentation of elongated cylindrical clouds. II - Polytropic clouds

Statistics – Computation

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Computational Astrophysics, Molecular Clouds, Nebulae, Polytropic Processes, Star Formation, Stellar Mass, Density Distribution, Interstellar Magnetic Fields, Interstellar Matter

Scientific paper

A numerical study of the fragmentation of elongated polytropic axially symmetric clouds is presented. Results are obtained for various ratios of length to diameter L/D, polytropic constant gamma, and initial Jeans number J0. Initial density perturbations on the axis of otherwise uniformly dense cylinders are introduced, and the maximum number of fragments Nf(max) that can form and grow for combinations of L/D, gamma, and J0 is derived. At fixed values of L/D and J0, Nf(max) decreases when gamma increases. Since the saturation value Nmax is independent of gamma, reaching saturation at high gamma requires a larger initial Jeans number. The number of fragments formed can exceed 2L/D for gamma less than 1. The implications of these results for the minimum stellar mass are discussed.

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