Molecular cloud collapse to stellar densities: models on moving geodesic vs. unstructured tetrahedron vs. nested meshes
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
https://iopscience.iop.org/article/10.1088/1742-6596/2028/1/012001/pdf
Reference26 articles.
1. Numerical Calculations of the Dynamics of a Collapsing Proto-Star;Larson;Monthly Notices of the Royal Astronomical Society,1969
2. The Jeans Condition and Collapsing Molecular Cloud Cores: Filaments or Binaries?;Boss;The Astrophysical Journal,2000
3. Resolution requirements for smoothed particle hydrodynamics calculations with self-gravity;Bate;Monthly Notices of the Royal Astronomical Society,1997
4. Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations;Bate;The Astrophysical Journal,1998
5. Collapse of a molecular cloud core to stellar densities: the formation and evolution of pre-stellar discs;Bate;Monthly Notices of the Royal Astronomical Society,2011
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