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Gas flow in Close Binary Star Systems

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New Developments in Computational Fluid Dynamics

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Summary

We first present a summary of our numerical work on accretion discs in close binary systems. Our recent studies on numerical simulations of the surface flow on the mass-losing star in a close binary star is then reviewed.

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Author information

Authors and Affiliations

  1. Department of Earth and Planetary Sciences, Kobe University, Kobe, 657-8501, Japan

    T. Matsuda1 & K. Oka1

  2. Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Komaba, Meguro-ku, Tokyo, 153-8902, Japan

    I. Hachisu

  3. European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748, Garching-bei-Muenchen, Germany

    H.M.J. Boffin

Authors
  1. T. Matsuda1
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  2. K. Oka1
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  3. I. Hachisu
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  4. H.M.J. Boffin
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Editor information

Editors and Affiliations

  1. Institute of Space and Astronautical Science (ISAS), Yoshinodai, Sagamihara 3-1-1, 229-8510, Kanagawa, Japan

    Kozo Fujii

  2. Department of Aeronautics/Space Engineering, Tohoku University, Katahira 1-1-2, 980-8577, Sendai, Japan

    Kazuhiro Nakahashi

  3. Institute of Fluid Science, Tohoku University, Katahira 2-1-1, 980, Sendai, Japan

    Shigeru Obayashi

  4. College of Science & Technology Department of Mathematics, Nihon University, Kanda-Surugadai 1-8, 101-0062, Tokyo, Japan

    Satoko Komurasaki

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© 2005 Springer-Verlag Berlin Heidelberg

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Matsuda1, T., Oka1, K., Hachisu, I., Boffin, H. (2005). Gas flow in Close Binary Star Systems. In: Fujii, K., Nakahashi, K., Obayashi, S., Komurasaki, S. (eds) New Developments in Computational Fluid Dynamics. Notes on Numerical Fluid Mechanics and Multidisciplinary Design (NNFM), vol 90. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-31261-7_18

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  • DOI: https://doi.org/10.1007/3-540-31261-7_18

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-27407-0

  • Online ISBN: 978-3-540-31261-1

  • eBook Packages: EngineeringEngineering (R0)

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