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Erratum: Detection of a second high-velocity component in the highly ionized wind from PG 1211+143

2016; Oxford University Press; Volume: 464; Issue: 2 Linguagem: Inglês

10.1093/mnras/stw2383

ISSN

1365-2966

Autores

Ken Pounds, A. Lobban, J. N. Reeves, S. Vaughan,

Tópico(s)

Pulsars and Gravitational Waves Research

Resumo

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 Xray observation of the Seyfert galaxy IRAS 17020+4544, indicating up to five outflow components with velocities in the range v ≈

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