Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-05-06
Mon.Not.Roy.Astron.Soc.352:744,2004
Astronomy and Astrophysics
Astrophysics
To appear in MNRAS. Submitted March 01, 2004. 9 pages
Scientific paper
10.1111/j.1365-2966.2004.08003.x
The narrow-line quasar PHL 1092 was observed by XMM-Newton at two epochs separated by nearly thirty months. Timing analyses confirm the extreme variability observed during previous X-ray missions. A measurement of the radiative efficiency is in excess of what is expected from a Schwarzschild black hole. In addition to the rapid X-ray variability, the short UV light curves (< 4 hours) obtained with the Optical Monitor may also show fluctuations, albeit at much lower amplitude than the X-rays. In general, the extreme variability is impressive considering that the broad-band (0.4-10 keV rest-frame) luminosity of the source is ~10^45 erg/s. During at least one of the observations, the X-ray and UV light curves show common trends, although given the short duration of the OM observations, and low significance of the UV light curves it is difficult to comment on the importance of this possible correlation. Interestingly, the high-energy photons (> 2 keV) do not appear highly variable. The X-ray spectrum resembles that of many narrow-line Seyfert 1 type galaxies: an intense soft-excess modelled with a multi-colour disc blackbody, a power-law component, and an absorption line at ~1.4 keV. The ~1.4 keV feature is curious given that it was not detected in previous observations, and its presence could be related to the strength of the soft-excess. Of further interest is curvature in the spectrum above ~2 keV which can be described by a strong reflection component. The strong reflection component, lack of high-energy temporal variability, and extreme radiative efficiency measurements can be understood if we consider gravitational light bending effects close to a maximally rotating black hole.
Boller Th.
Brandt Wiliam N.
Fabian Andrea C.
Gallo Luigi C.
Grupe Dirk
No associations
LandOfFree
An intense soft-excess and evidence for light bending in the luminous narrow-line quasar PHL 1092 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with An intense soft-excess and evidence for light bending in the luminous narrow-line quasar PHL 1092, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An intense soft-excess and evidence for light bending in the luminous narrow-line quasar PHL 1092 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-711816