Theory of Pulsar Wind Nebulae

@inproceedings{Bucciantini2008TheoryOP,
  title={Theory of Pulsar Wind Nebulae},
  author={N. Bucciantini},
  year={2008}
}
  • N. Bucciantini
  • Published 2008
  • Physics
  • Our understanding of Pulsar Wind Nebulae (PWNe), has greatly improved in the last years thanks to unprecedented high resolution images taken from the HUBBLE, CHANDRA and XMM satellites. The discovery of complex but similar inner features, with the presence of unexpected axisymmetric rings and jets, has prompted a new investigation into the dynamics of the interaction of the pulsar winds with the surrounding SNR, which, thanks to the improvement in the computational resources, has let to a… CONTINUE READING

    Create an AI-powered research feed to stay up to date with new papers like this posted to ArXiv

    Figures from this paper.

    References

    Publications referenced by this paper.
    SHOWING 1-7 OF 7 REFERENCES

    VHE gamma-ray emitting pulsar wind nebulae discovered by HESS

    • Y. A. Gallant, al
    • 2007
    VIEW 1 EXCERPT

    X-ray observation of pulsar tails

    • O. Kargaltsev, G. G. Pavolv, Z. Misanivic, G. P. Garmire
    • 2007
    VIEW 1 EXCERPT

    Thesis: “La Strutura Interna della Nebulosa del Granchio

    • D. Volpi
    • 2006
    VIEW 1 EXCERPT

    Neutron Star and Pulsar: Thirty years aft er Discovery

    • J. Arons
    • Proc. International Conference on Neutron Stars and Pulsars,
    • 1998
    VIEW 1 EXCERPT

    Neutron Star and Pulsar: Thirty years aft er Discovery

    • J. Arons
    • Proc. International Conference on Neutron Stars and Pulsars,
    • 1998
    VIEW 1 EXCERPT