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| Paper: |
MHD Simulation of Bondi–Hoyle Accretion onto Magnetized Neutron Star |
| Volume: |
459, 6th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM 2011) |
| Page: |
173 |
| Authors: |
Toropina, O. D.; Romanova, M. M.; Lovelacem R. V. E. |
| Abstract: |
Axisymmetric MHD simulations are used to investigate the
Bondi–Hoyle accretion onto an isolated magnetized neutron star
moving supersonically through the interstellar medium.
The star is assumed to have a dipole magnetic field
and a magnetospheric radius Rm less then the accretion
radius RBH, so that the gravitational focusing is
important. |
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