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| Paper: |
Magnetohydrodynamic Simulations of the Formation of Eruptive Magnetic Flux Ropes and Molecular Loops in the Galactic Center |
| Volume: |
528, New Horizons in Galactic Center Astronomy and Beyond |
| Page: |
135 |
| Authors: |
Tomiyoshi, T.; Matsumoto, R. |
| Abstract: |
We studied the formation mechanism of molecular loops in the galactic central region by three-dimensional magnetohydrodynamic simulations. The reconnection-condensation model of solar prominences has been extended to the galactic center by incorporating the interstellar cooling/heating. We found that dense, arch-like filaments are formed 100 pc above the galactic plane. |
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