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Propagation of Magnetized Neutron Stars Through the Interstellar Medium Authors: Toropina O.D., Romanova M.M., Toropin Yu.M., Lovelace R.V.E. |
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Propagation of Magnetized Neutron Stars Through the Interstellar Medium Authors: Toropina O.D., Romanova M.M., Toropin Yu.M., Lovelace R.V.E. |
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We
observed that accretion rate strongly decreases with increasing magnetic
field This dependence may reflect the fact that a stronger magnetic field
of the star deflects the incoming ISM flow more efficiently than weaker
magnetic field. From the other side, |
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Results
of simulations of motion of a magnetized star with magnetic field B*=14
through the ISM with Mach number M=3. Magnetic field lines and
velocity vectors are shown. The background represents the density. The
thick line indicates the Alfven surface. |
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Results
of simulations for M=10 and B*=14 |
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Results of simulations for M=50 and B*=14 |
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