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Title: Erratum: Detection of a second high-velocity component in the highly ionized wind from PG 1211+143
Authors: Pounds, Ken
Lobban, Andrew
Reeves, J.
Vaughan, Simon
First Published: 20-Sep-2016
Publisher: Oxford University Press (OUP), Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2016, 464 (2), pp. 2377-2377
Abstract: Three publications which were part of the accepted manuscript were omitted from the published version of the above paper (MNRAS 457, 2951, 2016). These are now added below, with the first two providing additional evidence for the existence of more complex structure in active galactic nuclei (AGN) winds. Gupta, Mathur & Krongold (2015) report a Chandra grating observation of the Seyfert galaxy Mrk 590, finding evidence for velocities v ≈ 0.074 c and v ≈ 0.176 c. Longinotti et al. (2015) report an XMM–Newton soft X-ray observation of the Seyfert galaxy IRAS 17020+4544, indicating up to five outflow components with velocities in the range v ≈ 0.079–0.113 c. Shih, Isasawa & Fabian (2002) is an early reference to a double power law being used in the study of spectral variability in AGN.
DOI Link: 10.1093/mnras/stw2383
ISSN: 0035-8711
eISSN: 1365-2966
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Creative Commons “Attribution Non-Commercial No Derivatives” licence CC BY-NC-ND, further details of which can be found via the following link: Archived with reference to SHERPA/RoMEO and publisher website.
Description: Correction to Pounds et al. 457 (3): 2951 doi: 10.1093/mnras/stw165
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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