Hostname: page-component-5c6d5d7d68-sv6ng Total loading time: 0 Render date: 2024-08-24T17:30:34.007Z Has data issue: false hasContentIssue false
  • English
  • Français

Multiple Gaseous Disks in NGC 1052

Published online by Cambridge University Press:  25 May 2016

H. Plana  and
J. Boulesteix
H. Plana
Affiliation:
Observatoire de Marseille 2 place Le Verrier F 13248
J. Boulesteix
Affiliation:
Observatoire de Marseille 2 place Le Verrier F 13248

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present detailed velocity field of NGC 1052 in [NII]6583Å line obtained with scanning Perot-Fabry. Extended ionized gas was studied by Davies et al. (1986) showing a clear counter-rotation between ionized gas and stars. It is an E4 galaxy type with ‘Boxy’ isophotes (Nieto et al. 1991). Taking benefit from high spectral resolution and 2D mapping of Scanning PF, we have discovered several components in our profiles (Plana 1995). Their study shows two main gaseous components: a first one with a Major Axis at PA=45° and a second one at PA=30°. The ionized gas extension is approximately 40″ for the first component and 20″ for the second. The main component contains 100 times more gas than the second one.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 432
Copyright
Copyright © Kluwer 1996 

References

Bertola, F. et al. 1991, ApJ, 373, 369.CrossRefGoogle Scholar
Davis, R. et al. 1986, ApJ, 302, 234.CrossRefGoogle Scholar
Nieto, J.L. et al. 1991, A&AS, 88, 559.Google Scholar
Plana, H. et al. 1995, A&A, in press.Google Scholar
de Zeeuw, T. et al. 1989, ApJ, 343, 617.CrossRefGoogle Scholar