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Core Collapse With Rotation And Neutron Star Formation

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Timing Neutron Stars

Part of the book series: NATO ASI Series ((ASIC,volume 262))

Abstract

Numerical simulations of the collapse of non-rotating and rotating cores of massive stars (M ≥ 8 M ⊙) are presented. After reviewing briefly the underlying physics the numerical results are discussed and possible consequences for neutron star formation are outlined.

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Author information

Authors and Affiliations

  1. Max-Planck-Institut für Physik und Astrophysik, Institut für Physik, Karl-Schwarzschild-Straße 1, D-8046, Garching b. München, Germany

    Ralph Mönchmeyer & Ewald Müller

Authors
  1. Ralph Mönchmeyer
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  2. Ewald Müller
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Editor information

Editors and Affiliations

  1. Max-Planck Institute for Extraterrestrial Physics, Garching, Germany

    H. Ögelman

  2. Astronomical Institute and Center for High-Energy Astrophysics, University of Amsterdam, Amsterdam, The Netherlands

    E. P. J. van den Heuvel

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© 1989 Kluwer Academic Publishers

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Mönchmeyer, R., Müller, E. (1989). Core Collapse With Rotation And Neutron Star Formation. In: Ögelman, H., van den Heuvel, E.P.J. (eds) Timing Neutron Stars. NATO ASI Series, vol 262. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2273-0_48

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  • DOI: https://doi.org/10.1007/978-94-009-2273-0_48

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7519-0

  • Online ISBN: 978-94-009-2273-0

  • eBook Packages: Springer Book Archive

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