Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-29T02:39:28.410Z Has data issue: false hasContentIssue false
  • English
  • Français

Predicted Fe I-III fluxes for AGNs with BLRs

Published online by Cambridge University Press:  01 December 2004

T. A. A. Sigut ,
Anil K. Pradhan  and
Sultana N. Nahar
T. A. A. Sigut
Affiliation:
Department of Physics & Astronomy, The University of Western Ontario, London, Ontario, Canada email: [email protected]
Anil K. Pradhan
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, Ohio, USA
Sultana N. Nahar
Affiliation:
Department of Astronomy, The Ohio State University, Columbus, Ohio, USA
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.

We present theoretical Fe I-III emission-line strengths for physical conditions typical of Active Galactic Nuclei with Broad-Line Regions. We can satisfactorily reproduce the empirical UV Fe II-III emission-line template of Vestergaard & Wilkes (2001) for the prototypical narrow-line Seyfert 1 galaxy I Zw 1, although a number of detailed discrepancies remain.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 363 - 364
Copyright
© 2004 International Astronomical Union