http://arxiv.org/abs/1910.14583
We present new XMM-Newton and NuSTAR observations of the galaxy merger IRAS F05189-2524 which is classified as an ultra-luminous infrared galaxy (ULIRG) and optical Seyfert 2 at $z$ = 0.0426. We test a variety of spectral models which yields a best-fit consisting of an absorbed power law with emission and absorption features in the Fe K band. Remarkably, we find evidence for a blueshifted Fe K absorption feature at $E$ = 7.8 keV (rest-frame) which implies an ultra-fast outflow (UFO) with $v_{\mathrm{out}} = 0.11\ \pm\ 0.01c$. We calculate that the UFO in IRAS F05189-2524 has a mass outflow rate of $\dot{M}{\mathrm{out}}\ \gtrsim 1.0\ M\odot$ yr$^{-1}$, a kinetic power of $\dot{E}{\mathrm{K}} \gtrsim$ 8% $L{\mathrm{AGN}}$, and a momentum rate (or force) of $\dot{P}{\mathrm{out}}\ \gtrsim 1.4\ L{\mathrm{AGN}}/c$. Comparing the energetics of the UFO to the observed multi-phase outflows at kiloparsec scales yields an efficiency factor of $f\sim0.05$ for an energy-driven outflow. Given the uncertainties, however, we cannot exclude the possibility of a momentum-driven outflow. Comparing IRAS F05189-2524 with nine other objects with observed UFOs and large-scale galactic outflows suggests that there is a range of efficiency factors for the coupling of the energetics of the nuclear and galaxy-scale outflows that likely depend on specific physical conditions in each object.
R. Smith, F. Tombesi, S. Veilleux, et. al.
Fri, 1 Nov 19
41/54
Comments: 23 pages, 8 figures; accepted by ApJ