Hostname: page-component-8448b6f56d-sxzjt Total loading time: 0 Render date: 2024-04-24T13:12:41.040Z Has data issue: false hasContentIssue false
  • English
  • Français

Infrared Line Shapes in Active Galactic Nuclei

Published online by Cambridge University Press:  19 July 2016

Rodger I. Thompson
Rodger I. Thompson*
Affiliation:
Steward Observatory, University of Arizona

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.

This paper presents the complete spectrum of NGC 4151 from 0.87 to 2.5 μm as well as detail of the Paschen α profile in 3C273 at a resolution of about 5000. Analysis of the several observed Fe II lines yields a most probable electron density of 104 and a most likely temperature of 104. The Fe II to H ratio is 2+/− 1 × 10−6 which is 5–7% of the available iron if the Fe/H ratio is solar.

Type
Poster Contributions: Line Studies
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 462
Copyright
Copyright © Kluwer 1994 

References

Osterbrock, D.E., Shaw, R.A., and Veilleux, S. 1992, Ap J. , 352, 561.Google Scholar
Pradhan, A.K. and Zhang, H.L. 1993, Ap J (Letters) , 409, L77.Google Scholar