Propagation of Magnetars through the Interstellar Medium

Details Propagation of Magnetars through the Interstellar Medium Propagation of Magnetars through the Interstellar Medium

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confq..95t&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 95-95"

Computer Science

Scientific paper

This work investigates the propagation of magnetars through the interstellar medium (ISM) using axisymmetric resistive magnetohydrodynamic simulations. We consider two cases: (1) Slow rotating magnetar, when the accretion radius R_{acc} is comparable to the magnetic standoff distance or Alfven radius R_A and gravitational focusing is important and (2) Magnetar rotating in the propeller regime, when accreting matter tends to be expelled from the equatorial region of the magnetosphere where the centrifugal force on matter corotating with the star exceeds the gravitational force.

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