3D Modelling of the interaction of Pulsar Wind Nebula (PWN) with Interstellar medium

ORAL

Abstract

We have investigated, in three dimensions, the interaction of the Pulsar Wind Nebulae (PWN) with an interstellar medium. We have considered the case of asymmetric wind luminosity and investigated its impact on the bow shock structure and other observables. Our results are compared to several observations.

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Authors

  • Tanvir Rahman

    Long Island University, McGill, Long Island University

  • David Neilsen

    Brigham Young University

  • Eric Hirschmann

    Brigham Young University

  • Steve Liebling

    Long Island University, C.W. Post -- Long Island University

  • Mallory Roberts

    Eureka Scientific