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- W2745698265 abstract "We present a newly discovered correlation between the wind outflow velocity and the X-ray luminosity in the luminous (Lbol ∼ 1047erg s − 1) nearby (z = 0.184) quasar PDS 456. All the contemporary XMM–Newton, NuSTAR and Suzaku observations from 2001–2014 were revisited and we find that the centroid energy of the blueshifted Fe K absorption profile increases with luminosity. This translates into a correlation between the wind outflow velocity and the hard X-ray luminosity (between 7 and 30 keV) where we find that |$v_{rm w}/cpropto L_{7-30}^{gamma }$| where γ = 0.22 ± 0.04. We also show that this is consistent with a wind that is predominately radiatively driven, possibly resulting from the high Eddington ratio of PDS 456." @default.
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- W2745698265 date "2017-08-16" @default.
- W2745698265 modified "2023-10-18" @default.
- W2745698265 title "Evidence for a radiatively driven disc-wind in PDS 456?" @default.
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- W2745698265 doi "https://doi.org/10.1093/mnrasl/slx129" @default.
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