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Galaxy Interactions at Low and High Redshift pp 135Cite as

Towards an Interaction Model of M81, M82 and Ngc 3077

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Part of the book series: International Astronomical Union ((IAUS,volume 186))

Abstract

Thomson (1992) suggested that the Cen A group of galaxies may be the result of one interaction. Here we report full N-body simulations made to study this proposal in the M81-M82-NGC 3077 group.

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Author information

Authors and Affiliations

  1. Department of Physical Sciences, University of Hertfordshire, Hatfield, Herts AL10 9AB, UK

    R. C. Thomson, S. Laine & A. Turnbull

Authors
  1. R. C. Thomson
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  2. S. Laine
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  3. A. Turnbull
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Editor information

Editors and Affiliations

  1. Institute for Astronomy, University of Hawaii, Honolulu, HI, USA

    J. E. Barnes  & D. B. Sanders  & 

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© 1999 Springer Science+Business Media Dordrecht

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Thomson, R.C., Laine, S., Turnbull, A. (1999). Towards an Interaction Model of M81, M82 and Ngc 3077. In: Barnes, J.E., Sanders, D.B. (eds) Galaxy Interactions at Low and High Redshift. International Astronomical Union, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4665-4_28

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  • DOI: https://doi.org/10.1007/978-94-011-4665-4_28

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-5833-6

  • Online ISBN: 978-94-011-4665-4

  • eBook Packages: Springer Book Archive

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