Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-27T07:23:32.551Z Has data issue: false hasContentIssue false
  • English
  • Français

Highly Ionized Gas as a Diagnostic of the Inner NLR

Published online by Cambridge University Press:  03 June 2010

M. J. Ward ,
J. Mullaney ,
C. Jin  and
R. Davies
M. J. Ward
Affiliation:
Department of Physics, Durham University, Durham, UK
J. Mullaney
Affiliation:
Department of Physics, Durham University, Durham, UK
C. Jin
Affiliation:
Department of Physics, Durham University, Durham, UK
R. Davies
Affiliation:
Max-Planck Institut für extraterrestrische Physik, Garching, Germany
Rights & Permissions [Opens in a new window]

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.

The spectra of AGN, from the ultraviolet to the near infrared, exhibit emission lines covering a wide range of ionization states, from neutral species such as [O i] λ 6300, up to [Fe iv] λ 5303. Here we report on some recent studies of the properties of highly ionized lines (HILs), plus two case studies of individual objects. Future IFU observations at high spatial and good spectral resolution will probe the excitation and kinematics of the gas in the zone between the extended NLR and unresolved BLR. Multi-component SED fitting can be used to link the source of photoionization with the strengths and ratios of the HILs.

Keywords

galaxies: activegalaxies: kinematics and dynamicsgalaxies: nucleigalaxies: Seyfert
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 383 - 386
Copyright
Copyright © International Astronomical Union 2010

References

Ferguson, J., Korista, K., & Ferland, G. 1997, ApJS, 110, 287CrossRefGoogle Scholar
Gelbord, J., Mullaney, J. R., & Ward, M. 2009, MNRAS, 397, 172CrossRefGoogle Scholar
Landt, H., Bentz, M., Ward, M., Elvis, M., Peterson, B. M., Korista, K., & Karovska, M. 2008, ApJS, 174, 282CrossRefGoogle Scholar
Marconi, A., van der Werf, P., Moorwood, A., & Oliva, E. 1996, A&A, 315, 335Google Scholar
Mazzalay, X., Rodriguez-Ardila, A., & Komossa, S. 2010, MNRAS, in press [arXiv:1002.3152]Google Scholar
Mullaney, J. R. & Ward, M. 2008, MNRAS, 385, 53CrossRefGoogle Scholar
Mullaney, J., Ward, M., Done, C., Ferland, G., & Schurch, N. 2010, MNRAS, 394, L16CrossRefGoogle Scholar
Pelat, D., Alloin, D., & Fosbury, R. 1981, MNRAS, 195, 787CrossRefGoogle Scholar
Penston, M., Fosbury, R., Boksenberg, A., Ward, M., & Wilson, A. 1984, MNRAS, 208, 364CrossRefGoogle Scholar
Prieto, M. A., Marco, O., & Gallimore, J. 2005, MNRAS, 364, L28CrossRefGoogle Scholar
Reeves, J., O'Brien, P., Braito, V., Behar, E., Miller, L., Turner, T., Fabian, A., Kaspi, S., Mushotzky, R., & Ward, M. 2009, ApJ, 701, 493CrossRefGoogle Scholar
Riffel, R., Rodriquez-Ardilla, A., & Pastoriza, M. 2006, A&A, 457, 61Google Scholar
Rodriguez-Ardila, A., Prieto, M., Viegas, S., & Gruenwald, R. 2006, ApJ, 653, 1098CrossRefGoogle Scholar