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Pulsar-Wind Nebulae

Recent Progress in Observations and Theory

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The Strongest Magnetic Fields in the Universe

Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 54))

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Abstract

In this review we describe recent observational and theoretical developments in our understanding of pulsar winds and pulsar-wind nebulae (PWNe). We put special emphasis on the results from observations of well-characterized PWNe of various types (e.g., torus-jet and bowshock-tail), the most recent MHD modeling efforts, and the status of the flaring Crab PWN puzzle.

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Authors and Affiliations

  1. George Washington University, 105 Corcoran Hall, Washington DC, 20052, USA

    Oleg Kargaltsev

  2. Department of Astrophysical Sciences, Princeton University, Princeton, NJ, 08544, USA

    Benoît Cerutti

  3. Ben-Gurion University, P.O. Box 653, Beer-Sheva, 84105, Israel

    Yuri Lyubarsky

  4. Department of Physics, University of Torino, Via P. Giuria 1, 10125, Turin, Italy

    Edoardo Striani

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  4. Edoardo Striani
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  1. Russian Academy of Sciences, Moscow, Russia

    V.S. Beskin

  2. The Blackett Laboratory, Imperial College London, London, United Kingdom

    A. Balogh

  3. International Space Science Institute, Bern, Switzerland

    M. Falanga

  4. Purdue University, West Lafayette, Indiana, USA

    M. Lyutikov

  5. INAF-IASF Milano, Milano, Italy

    S. Mereghetti

  6. The Hebrew University, Racah Institute for Physics, Jerusalem, Israel

    T. Piran

  7. International Space Science Institu, Bern, Switzerland

    R.A. Treumann

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Kargaltsev, O., Cerutti, B., Lyubarsky, Y., Striani, E. (2016). Pulsar-Wind Nebulae. In: Beskin, V., et al. The Strongest Magnetic Fields in the Universe. Space Sciences Series of ISSI, vol 54. Springer, New York, NY. https://doi.org/10.1007/978-1-4939-3550-5_12

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