Stephan’s Quintet Revisited

  • J. M. van der Hulst
  • A. H. Rots
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 97)

Abstract

VLA observations at 1465 MHz of the Stephan’s Quintet region reveal that the arc-shaped area of emission discussed by Allen and Hartsuiker (1972) breaks up into several components. The idea that NGC 7318b is a recent interloper in the group and that the interaction resulting from this event causes the enhanced activity at the east side of NGC 7318b is adopted as still the most reasonable explanation. The results are discussed in more detail in another paper (van der Hulst and Rots, 1981).

References

  1. Allen, R.J. and Hartsuiker, J.W. 1972, Nature 239, p. 324.ADSCrossRefGoogle Scholar
  2. Allen, R.J. and Sullivan, W.T. 1980, Astron. Astrophys. 84, p. 181.ADSGoogle Scholar
  3. Arp, H.C. 1973, Astrophys. J. 183, p. 411.ADSCrossRefGoogle Scholar
  4. Peterson, S.D. and Shostak, G.S. 1980, Astrophys. J. 241, p. L1.ADSCrossRefGoogle Scholar
  5. van der Hulst, J.M. and Rots, A.H. 1981, Astron. J. (in press).Google Scholar

Copyright information

© IAU 1982

Authors and Affiliations

  • J. M. van der Hulst
    • 1
  • A. H. Rots
    • 2
  1. 1.Department of AstronomyUniversity of MinnesotaMinneapolisUSA
  2. 2.National Radio Astronomy ObservatorySocorroUSA

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