Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-17T23:37:15.489Z Has data issue: false hasContentIssue false
  • English
  • Français

Bidimensional [O III] λλ4959, 5007 Spectroscopy in the Circumnuclear Region of the Active Galaxy NGC 1068

Published online by Cambridge University Press:  12 April 2016

B. García-Lorenzo ,
S. Arribas ,
E. Mediavilla  and
C. del Burgo
B. García-Lorenzo
Affiliation:
Instituto de Astrofisica de Canarias, 38200–La Laguna, Tenerife, Spain
S. Arribas
Affiliation:
Instituto de Astrofisica de Canarias, 38200–La Laguna, Tenerife, Spain
E. Mediavilla
Affiliation:
Instituto de Astrofisica de Canarias, 38200–La Laguna, Tenerife, Spain
C. del Burgo
Affiliation:
Instituto de Astrofisica de Canarias, 38200–La Laguna, Tenerife, Spain

Abstract

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 preliminary results about the velocity field of the ionized gas in the central region of NGC 1068, inferred from the [O III] λλ4959, 5007 emission lines. The data, 570 spectra in the inner 23″ × 18″ of this galaxy, were obtained with an optical fiber system which allows 2-D spectroscopy. The velocity field for the ionized gas inferred from the [O III] lines is in good agreement with recent results based on the Hα+[N II] lines.

Type
VI. The Narrow-Line Regions and Beyond
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 361 - 362
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Arribas, S., Mediavilla, E., & García-Lorenzo, B. 1996, ApJ, 463, 509.CrossRefGoogle Scholar
Cecil, G., Bland, J., & Tully, R.B. 1990, ApJ, 355, 70.CrossRefGoogle Scholar
García, A., Rasilla, J.L., Arribas, S., & Mediavilla, E. 1994, SPIE, Vol 2198, 75.Google Scholar
Kaneko, N., Satoh, T., Toyama, K., Sasaki, M., Nishimura, M., & Yamamoto, M. 1992, PASJ, 44, 341.Google Scholar