3D MHD Modeling of the Gaseous Structure of the Galaxy.

@inproceedings{Gomez20023DMM,
  title={3D MHD Modeling of the Gaseous Structure of the Galaxy.},
  author={G. Gomez and Donald P. Cox},
  year={2002}
}
We show the results of our 3D MHD simulations of the o w of the Galactic atmosphere as it responds to a spiral perturbation in the potential. 
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    Publications of the Astronomical Society of Japan
  • 2018
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