University of Hertfordshire

M100 and NGC 6951: Morphological Clues to Central Dynamics

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

  • J. Knapen
  • I. Shlosman
  • J.E. Beckman
  • C.H. Heller
  • R.F. Peletier
  • R.S. de Jong
  • D. Nadeau
  • R. Doyon
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Original languageEnglish
Title of host publicationIn: Barred galaxies, ASP Conference Series 91
PublisherAstronomical Society of the Pacific
Pages416-9
ISBN (Print)1-886733-12-0
Publication statusPublished - 1996

Abstract

High-resolution optical and NIR observations are used to constrain a dynamical model of the circumnuclear star forming (SF) region in the barred galaxy M100 (NGC 4321). Small leading arms observed in our K-band image of the nuclear region have been reproduced in numerical modeling of M100, a galaxy with a double inner Lindblad resonance (ILR). We also present preliminary optical and NIR observations of NGC 6951: a barred galaxy with circumnuclear SF showing a distinctly different behavior to M100 at 2.2um.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific

ID: 179684