Using Ark 564 and I Zw 1 as Laboratories for Modeling the Fe II Pseu0do-Continuum in QSOs
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.
- Publication:
-
Co-Evolution of Central Black Holes and Galaxies
- Pub Date:
- May 2010
- DOI:
- 10.1017/S174392131000637X
- Bibcode:
- 2010IAUS..267..260E
- Keywords:
-
- accretion disks;
- quasars: emission lines;
- galaxies: Seyfert;
- atomic processes