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Evolution of close binaries and gamma-ray bursts

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Abstract

We analyze the late stages of evolution of massive (M 0 ≳ 8 M ⊙) close binaries, from the point of view of possible mechanisms for the generation of gamma-ray bursts. It is assumed that a gamma-ray burst requires the formation of a massive (∼1 M ⊙), compact (R ≲ 10 km) accretion disk around a Kerr black hole or neutron star. Such Kerr black holes are produced by core collapses of Wolf-Rayet stars in very close binaries, as well as by mergers of neutron stars and black holes or two neutron stars in binaries. The required accretion disks can also form around neutron stars that were formed via the collapse of ONeMg white dwarfs. We estimate the Galactic rate of events resulting in the formation of rapidly rotating relativistic objects. The computations were carried out using the “Scenario Machine.”

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Authors and Affiliations

  1. Institute of Applied Mathematics, Moscow, Russia

    A. I. Bogomazov

  2. Sternberg Astronomical Institute, Moscow State University, Moscow, Russia

    V. M. Lipunov

  3. Institute of Astronomy, Moscow, Russia

    A. V. Tutukov

Authors
  1. A. I. Bogomazov
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  2. V. M. Lipunov
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  3. A. V. Tutukov
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Original Russian Text © A.I. Bogomazov, V.M. Lipunov, A.V. Tutukov, 2007, published in Astronomicheskiĭ Zhurnal, 2007, Vol. 84, No. 4, pp. 345–356.

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Bogomazov, A.I., Lipunov, V.M. & Tutukov, A.V. Evolution of close binaries and gamma-ray bursts. Astron. Rep. 51, 308–317 (2007). https://doi.org/10.1134/S1063772907040063

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