Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-24T15:50:58.544Z Has data issue: false hasContentIssue false
  • English
  • Français

A Unified View of NGC 4151

Published online by Cambridge University Press:  19 July 2016

Hartmut Schulz
Hartmut Schulz*
Affiliation:
Radioastronomisches Institut, Universität Bonn, Auf dem Hügel 71, D-53121 Bonn and Astronomisches Institut, Ruhr-Universität, D-44780 Bochum

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.

Using crude constraints from recent HST images, we fit the emission-line spectra of the NLR and VNLR of NGC 4151 with photoionization models. There is no need for an intrinsic anisotropy of the distribution of the ionizing flux.

Type
Poster Contributions: Line Studies
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 458
Copyright
Copyright © Kluwer 1994 

References

Boksenberg, A., 1992, ESO Conf. Proc. 44, p.61 Google Scholar
Evans, I.N. et al., 1993, ApJ., in press Google Scholar
Ferland, G., 1993, Univ. Ky. Dep. Phys. & Astron. Int. Report Google Scholar
Schulz, H., 1988, A&A, 203, 233 Google Scholar
Schulz, H., 1990, AJ, 99, 1442 Google Scholar
Schulz, H., Komossa, S., 1993, A&A, in press Google Scholar