Letter | Published:

Acceleration of pulsars to high velocities by asymmetric radiation

Abstract

HERE we propose that pulsars are accelerated by the emission of asymmetric low frequency electromagnetic radiation and rapidly attain characteristic velocities exceeding 100 km s−1.

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References

  1. 1

    Ostriker, J. P., and Gunn, J. E., Astrophys. J., 157, 1395 (1969).

  2. 2

    Preston, G. W., IAU Symp. Stellar Rotation (edit. by Slettebak, A.), 254 (Reidel, Dordrecht, 1970).

  3. 3

    Stift, M. J., Mon. Not. R. astr. Soc., 169, 471 (1974).

  4. 4

    Backer, D. C., Boriakoff, V., and Manchester, R. N., Nature, 243, 77 (1973).

  5. 5

    Manchester, R. N., Science, 186, 66 (1974).

  6. 6

    Manchester, R. N., Taylor, J. H., and Van, Y. Y., Astrophys. J. Lett., 189, L119 (1974).

  7. 7

    Trimble, V., and Rees, M. J., Astrophys. J. Lett., 166, L85 (1971).

  8. 8

    Hulse, R. A., and Taylor, J. H., Astrophys. J. Lett., 195, L51 (1975).

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