Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 399, Issue 1, Pages L169-L173Publisher
OXFORD UNIV PRESS
DOI: 10.1111/j.1745-3933.2009.00746.x
Keywords
accretion, accretion discs; galaxies: active; galaxies: individual: 1H0707-495; quasars: emission lines; X-rays: galaxies
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Funding
- STFC
- Royal Society
- Science and Technology Facilities Council [PP/D003636/2] Funding Source: researchfish
- STFC [PP/D003636/2] Funding Source: UKRI
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We use a 380-ks X-ray Multi-Mirror Mission-Newton (XMM-Newton) high-resolution Reflection Grating Spectrometer (RGS) spectrum to look for narrow spectral features from the nuclear environment of 1H0707-495. We do not find any evidence of a line-of-sight ionized wind (warm absorber). We do, however, detect broad emission lines, of width similar to 5000 km s(-1), consistent with O VIII Ly alpha, N VII Ly alpha, C VI Ly alpha and an Fe XIX/Fe XX/Ne IX He alpha blend. Intriguingly, these lines have both blueshifted and redshifted components, whose velocity shifts are consistent with an origin in an accretion disc at similar to 1600 R-g from the black hole. The features can be interpreted as the narrow-line cores of the disc reflection spectrum, thus providing independent support for the discline interpretation of the X-ray spectrum of 1H0707-495. We discuss the relevance of our findings for the 'X-ray broad-line region' in other Seyferts, and for the origins of the optical broad-line region itself.
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