Stochastic spin evolution of neutron stars

Preprint English OPEN
Popov, S. B.; Prokhorov, M. E.; Khoperskov, A. V.; Lipunov, V. M.;
(2001)
  • Subject: Astrophysics
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::High Energy Astrophysical Phenomena | Astrophysics::Cosmology and Extragalactic Astrophysics

In this paper we present calculations of period distribution for old accreting isolated neutron stars (INSs). At the age about a few billions years low velocity INSs come to the stage of accretion. At that stage their period evolution is governed by magnetic breaking an... View more
  • References (9)

    1 Colpi M., Possenti A., Popov S.B., Pizzolato F.: 2001, in 'Physics of Neutron Star Interiors”, Eds. D. Blaschke, N.K. Glendenning, & A. Sedrakian (Springer-Verlag, Berlin), (astro-ph/0012394)

    2 Ghosh, P., & Lamb, F.K. 1979, ApJ 232, 256

    3 Konenkov, D.Yu., & Popov, S.B. 1997, PAZh, 23, 569

    4 Lipunov, V.M., 1992, “Astrophysics of Neutron Stars”, Springer-Verlag (Berlin)

    5 Lipunov, V.M., & Popov, S.B. 1995a, AZh, 72, 711

    6 Lipunov, V.M., & Popov, S.B. 1995b, Astron. Astroph. Transactions, 8, 221

    7 Motch, C. 2000, astro-ph/0008485

    8 Prokhorov, M.E., Popov, S.B., & Khoperskov, A.V. 2001, astro-ph/0108503

    9 Treves, A., Turolla, R., Zane, S., & Colpi, M. 2000, PASP 112, 297

  • Metrics
Share - Bookmark