Abstract
We present a spectral analysis of the narrow-line Seyfert 1 galaxy I Zwicky 1, focusing
on the characteristics of the ionised absorbers as observed with XMM-Newton in 2005.
The outflow
velocity of the X-ray low-ionisation absorber is consistent with the outflow of the UV
absorber detected in a past Hubble Space Telescope observation. In addition, the ionic
column densities of Civ and Nv derived from the X-ray model are consistent with
the UV values. This suggests that the low-ionisation outflowing gas may survive for
many years, despite large changes in flux, and that there is a tight connection between
the X-ray and UV absorbers that can only be confirmed with a simultaneous UV and
X-ray observation.
Original language | Undefined/Unknown |
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Pages (from-to) | 873-880 |
Number of pages | 8 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 378 |
Issue number | 3 |
Publication status | Published - 2007 |