University of Hertfordshire

Interaction Between NGC 5394 and NGC 5395

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

Documents

  • M. Kaufman
  • E. Brinks
  • B. Elmegreen
  • D.M. Elmegreen
  • M. Klaric
  • C. Struck
  • M. Thomasson
  • S. Vogel
View graph of relations
Original languageEnglish
Title of host publicationIn: Galaxy Dynamics, ASP Conf Series 182
PublisherAstronomical Society of the Pacific
Pages453-5
Publication statusPublished - 1999

Abstract

The spiral galaxies NGC 5394/95 (at a distance of 47 Mpc) are involved in a recent, close, nonmerging encounter. The smaller galaxy, NGC 5394, has two long, fairly symmetric, open tidal arms (see Figure 1); in numerical simulations, this type of structure results from a close, prograde, nearly in-plane encounter. To study this galaxy pair, we used the VLA to obtain HI (21 cm line) and radio continuum data, the Maryland-Caltech Fabry-Perot camera to obtain Ha data, the 2.1m telescope at KPNO, the Fick observatory 0.6 m telescope, and the Burrell-Schmidt telescope to take optical and near-infrared images, and Onsala Space Observatory for CO J=1-0 observations.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific

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