Using Ark 564 and I Zw 1 as Laboratories for Modeling the Fe II Pseu0do-Continuum in QSOs

Details Using Ark 564 and I Zw 1 as Laboratories for Modeling the Fe II Pseu0do-Continuum in QSOs Using Ark 564 and I Zw 1 as Laboratories for Modeling the Fe II Pseu0do-Continuum in QSOs

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..260e&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Astronomy and Astrophysics

Astronomy

Accretion Disks, Quasars: Emission Lines, Galaxies: Seyfert, Atomic Processes

Scientific paper

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.

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