Stellar Systems, Galaxy, Extragalactic Objects, Cosmology

  • S. Böhme
  • W. Fricke
  • H. Hefele
  • I. Heinrich
  • W. Hofmann
  • D. Krahn
  • V. R. Matas
  • L. D. Schmadel
  • G. Zech
Part of the Astronomy and Astrophysics Abstracts book series (AAA, volume 31)

Abstract

The authors describe the stationary states of motion of gas in a triaxial stellar system which rotates about one of its principal axes. Four dynamically different situations are possible, in two of these the gas layer is warped. The morphology of elliptical radio galaxies with dust lanes such as NGC 5128 (Cen A) and M 84 can be understood on the basis of this model; transient phenomena are not required.

Keywords

Torque Recombination Recent Epoch Reso Deconvolution 

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Copyright information

© Springer-Verlag Berlin Heidelberg 1982

Authors and Affiliations

  • S. Böhme
  • W. Fricke
  • H. Hefele
  • I. Heinrich
  • W. Hofmann
  • D. Krahn
  • V. R. Matas
  • L. D. Schmadel
  • G. Zech

There are no affiliations available

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