Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S267(5), p. 260-260, 2009
DOI: 10.1017/s174392131000637x
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Using Ark 564 and I Zw 1 as Laboratories for Modeling the Fe II Pseu0do-Continuum in QSOs
Journal article published in 2009 by
R. T. Eufrasio 
,
F. Bruhweiler,
E. Verner,
B. Wills,
D. M. Crenshaw
,
F. Bruhweiler,
E. Verner,
B. Wills,
D. M. Crenshaw
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Abstract
In this work, we use the low-redshift, narrow-line Seyfert 1 (NLS1) galaxies Ark 564 and I Zw 1 as laboratories for modeling the Fe ii emission features in the wavelength range 1200–6700 Å. We utilize data acquired with the Hubble Space Telescope and the 2.7-m telescope at McDonald Observatory.
