(Q56003523)

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Star formation with 3-D adaptive mesh refinement: the collapse and fragmentation of molecular clouds

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Star formation with 3-D adaptive mesh refinement: the collapse and fragmentation of molecular clouds (English)

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author name string

Richard I. Klein

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1

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publication date

September 1999

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published in

Journal of Computational and Applied Mathematics

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volume

109

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issue

1-2

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page(s)

123-152

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Local adaptive mesh refinement for shock hydrodynamics

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Formation of hierarchical multiple protostellar cores

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Collapse and fragmentation of molecular cloud cores. IV. Oblate clouds and small cluster formation

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The Piecewise Parabolic Method (PPM) for gas-dynamical simulations

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A production mechanism for clusters of dense cores

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The Stability of a Spherical Nebula

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A comparison of cosmological hydrodynamic codes

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On the hydrodynamic interaction of shock waves with interstellar clouds. I. Nonradiative shocks in small clouds

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Bending mode instabilities and fragmentation in interstellar cloud collisions: a mechanism for complex structure

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Collapse and fragmentation models of prolate molecular cloud cores. I. Initial uniform rotation

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Self-gravitational hydrodynamics with three-dimensional adaptive mesh refinement: methodology and applications to molecular cloud collapse and fragmentation

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X-ray-heated coronae and winds from accretion disks: time-dependent two-dimensional hydrodynamics with adaptive mesh refinement

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Identifiers

DOI

10.1016/S0377-0427(99)00156-9

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zbMATH Open document ID

0946.76059

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(Q56003523)

Star formation with 3-D adaptive mesh refinement: the collapse and fragmentation of molecular clouds

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