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Simulation of Jet Formation from Magnetized Accretion Disk Around Kerr Black Hole

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Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology

Part of the book series: ESO ASTROPHYSICS SYMPOSIA ((ESO))

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Abstract.

We present a general relativistic magnetohydrodynamic simulation of jet formation from accretion disk around Kerr black hole.

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Authors and Affiliations

  1. Department of Engineering, Toyama University, 3190 Gofuku, Toyama 930-8555, Japan

    Shinji Koide

  2. Kwasan and Hida Observatory, Kyoto University, Yamashina, Kyoto 607-8471, Japan

    Kazunari Shibata

  3. National Astronornical Observatory, Mitaka, Tokyo 181-8588, Japan

    Takahiro Kudoh

  4. Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA

    David L. Meier

Authors
  1. Shinji Koide
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  2. Kazunari Shibata
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  3. Takahiro Kudoh
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  4. David L. Meier
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Editor information

Marat Gilfanov Rashid Sunyeav Eugene Churazov

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Koide, S., Shibata, K., Kudoh, T., Meier, D.L. Simulation of Jet Formation from Magnetized Accretion Disk Around Kerr Black Hole. In: Gilfanov, M., Sunyeav, R., Churazov, E. (eds) Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10856495_66

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  • DOI: https://doi.org/10.1007/10856495_66

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-43769-7

  • Online ISBN: 978-3-540-48014-3

  • eBook Packages: Springer Book Archive

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