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NGC 2188: A Case Study for Disk-Halo Interaction

  • H. Domgörgen
  • M. Dahlem
  • R.-J. Dettmar
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 171)

Abstract

A deep Hα image of the nearly edge-on (i ~ 86°; Tully, 1988) irregular galaxy NGC 2188 shows the presence of spectacular filaments of ionized gas extending from a large star-forming complex several hundred pc into the halo of the galaxy (Dettmar, 1994). The origin and ionization mechanism of such extraplanar diffuse ionized features is not yet clear. One promising idea is that the extraplanar DIG is due to large scale mass circulation, i.e. a galactic “fountain” (Shapiro & Field, 1976) or “chimney” (Norman & Ikeuchi, 1989). Hα filaments could then be the photoionized walls of such chimneys or fountains.

References

  1. Dettmar R.-J. 1994, in The Physics of the Interstellar Medium and Intergalactic Medium, PASP Conf. Series Vol. 80, Eds: Ferrara A. et al., p. 398Google Scholar
  2. Norman C.A., Ikeuchi S. 1989, ApJ 345, 372ADSCrossRefGoogle Scholar
  3. Shapiro P.R., Field G.B. 1976, ApJ 158, 279Google Scholar
  4. Tully R.B. 1988, Nearby Galaxy Catalog, Cambridge University PressGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1996

Authors and Affiliations

  • H. Domgörgen
    • 1
  • M. Dahlem
    • 2
  • R.-J. Dettmar
    • 3
  1. 1.Sternwarte der Universität BonnGermany
  2. 2.Space Telescope Science InstituteUSA
  3. 3.Astronomisches Institut der Universität BochumGermany

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