Multiwavelength campaign on Mrk 509. III. The 600 ks RGS spectrum: unravelling the inner region of an AGN
R. G. Detmers, J. S. Kaastra, K. C. Steenbrugge, J. Ebrero, G. A., Kriss, N. Arav, E. Behar, E. Costantini, G. Branduardi-Raymont, M. Mehdipour,, S. Bianchi, M. Cappi, P.-O. Petrucci, C. Pinto, E. M. Ratti, T. Holczer

TL;DR
This study analyzes a 600 ks high-resolution X-ray spectrum of Mrk 509, revealing detailed properties of its ionized outflow, emission lines, and ionization structure, providing new insights into the AGN's inner region.
Contribution
It presents the first demonstration that the ionized outflow in Mrk 509 consists of discrete ionization components rather than a smooth distribution, based on high-quality spectral data.
Findings
Ionized outflow has two velocity components at -13 km/s and -319 km/s.
Outflow shows four orders of magnitude in ionization parameter.
Ionization structure features two strong, discrete peaks.
Abstract
We present the results of our 600 ks RGS observation as part of the multiwavelength campaign on Mrk 509. The very high quality of the spectrum allows us to investigate the ionized outflow with an unprecedented accuracy due to the long exposure and the use of the RGS multipointing mode. We detect multiple absorption lines from the interstellar medium and from the ionized absorber in Mrk 509. A number of emission components are also detected, including broad emission lines consistent with an origin in the broad line region, the narrow OVII forbidden emission line and also (narrow) radiative recombination continua. The ionized absorber consists of two velocity components (v = -13 \pm 11 km/s and v = -319 \pm 14 km/s), which both are consistent with earlier results, including UV data. There is another tentative component outflowing at high velocity, -770 \pm 109 km/s, which is only seen in…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Astrophysical Phenomena and Observations
