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[ascl:1105.012] Stagger: MHD Method for Modeling Star Formation

Stagger is an astrophysical MHD code actively used to model star formation. It is equipped with a multi-frequency radiative transfer module and a comprehensive equation of state module that includes a large number of atomic and molecular species, to be able to compute realistic 3-D models of the near-surface layers of stars. The current version of the code allows a discretization that explicitly conserves mass, momentum, energy, and magnetic flux. The tensor formulation of the viscosity ensures that the viscous force is insensitive to the coordinate system orientation, thereby avoiding artificial grid-alignment.

Code site:
https://starformation.hpc.ku.dk/?q=node/18
Used in:
http://adsabs.harvard.edu/abs/2009ApJ...702L..37L http://adsabs.harvard.edu/abs/2007ApJ...661..972P
Bibcode:
2011ascl.soft05012G

Views: 1738

ascl:1105.012
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