A high velocity component to the complex absorption in IRAS 13349+2438
arXiv:1807.06310 · doi:10.1093/mnras/sty2020
Abstract
We present an analysis of XMM-Newton spectra of the low-redshift quasar IRAS 13349+2438. The RGS spectrum shows a large number of absorption lines from two zones of warm absorption, with velocities of -600 km s, as noted by previous authors. Additionally, we find robust evidence from multiple Lyα absorption lines for a previously undiscovered ultra-fast zone of absorption, with an outflow velocity of . The warm absorbers and ultra-fast outflow have similar mass outflow rates, around 40% of the Eddington accretion rate, but the kinetic power is dominated by the high velocity gas, which has a power of 4% of the Eddington luminosity.
arXiv comment13 pages, 13 figures, accepted for publication in MNRAS
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