Kinematics of Interacting Galaxies VV 317: Motions in the Bar of One of the Components

  • V. P. Arkhipova
  • V. L. Afanasiev
  • A. N. Burenkov
  • O. K. Sil’chenko
  • A. V. Zasov

Abstract

The pair of interacting galaxies VV 317 presents a divided system consisting of two galaxies of type Sc-Scd (for the photograph — see [1]). VV317a, mpg=14.8 [2], is a spiral galaxy of type SBc seen face-on. The short broad arms emerge from the ends of the bright bar. The structure of the galaxy disk is of c-d type, it contains small bright HII-regions and a lot of dust.

Keywords

Dust Depression 

References

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Copyright information

© Springer-Verlag Berlin Heidelberg 1990

Authors and Affiliations

  • V. P. Arkhipova
    • 1
  • V. L. Afanasiev
    • 2
  • A. N. Burenkov
    • 2
  • O. K. Sil’chenko
    • 1
    • 2
  • A. V. Zasov
    • 1
  1. 1.Sternberg Astronomical InstituteMoscowUSSR
  2. 2.Special Astrophysical ObservatoryNizhnij ArkhyzUSSR

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