The problem of the Fe II template in AGNs

Details The problem of the Fe II template in AGNs The problem of the Fe II template in AGNs

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pobeo..73..207p&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 73, p. 207 - 210 (2002). In: Proceedings of the T

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Iron Lines

Scientific paper

In order to make a template for fitting and subtracting the Fe II emission lines in the Hβ wavelength range, we applied an approximate relation for the Fe II line relative intensities as a function of temperature. Using the obtained relative intensities we fitted the Hβ wavelength range of several AGNs. We found a good fit of the redshelf of Hβ wavelength range of several AGNs. We found a good fit of the redshelf of Hβ with our Fe II template.

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