Implications of the Discovery of Millisecond Pulsar in SN 1987A

Preprint English OPEN
Nagataki, S.; Sato, K.;
(2000)
  • Identifiers: doi: 10.1143/PTP.105.429
  • Subject: Astrophysics
    arxiv: Astrophysics::High Energy Astrophysical Phenomena | Astrophysics::Instrumentation and Methods for Astrophysics

From the observation of a millisecond pulsar in SN 1987A, the following implications are obtained. 1) The pulsar spindown in SN 1987A is caused by radiating gravitational waves rather than by magnetic dipole radiation and/or relativistic pulsar winds. 2) A mildly deform... View more
  • References (28)
    28 references, page 1 of 3

    [1] S. Kumagai, T. Shigeyama, K. Nomoto, M. Hashimoto, and S. Itho, Astron. and Astropys. 273 (1993), 153.

    [2] S. Yamada and K. Sato, Astrophys. J. 434 (1994), 268.

    [3] M. Hashimoto, Prog. Theor. Phys. 94 (1995), 663.

    [4] S. Nagataki, Astrophys. J. Suppl. 127 (2000), 141.

    [5] J. Middleditch, J. A. et al., New Astronomy 5 (2000), 243 (astro-ph/0010044).

    [8] A. M. Soderberg, P. Challis and N. B. Suntzeff, American Astronomical Society Meeting 194 (1999), 8612.

    [9] B. M. Gaensler, R. N. Manchester, L. Staveley-Smith, A. K. Tzioumis, J. E. Reynoulds and M. J. Kesteven, Astrophys. J. 479 (1997), 845.

    [10] McCall and L. Marshall, Astrophys. J. 417 (1993), 75.

    [11] D. N. Burrows, E. Michael, U. Hwang, R. McCray, R. A. Chevalier, R. Petre, G. P. Garmine, S. S. Holt and J. A. Nousek, Astrophys. J. 543 (2000), 149.

    [12] C. Fransson and R. A. Chevalier, Astrophys. J. 322 (1987), L15.

  • Metrics
Share - Bookmark