The hard X-ray spectrum of NGC 1365: scattered light, not black hole spin
Active Galactic Nuclei (AGN) show excess X-ray emission above 10 keV compared with extrapolation of spectra from lower energies. Risaliti et al. have recently attempted to model the hard X-ray excess in the type 1.8 AGN NGC 1365, concluding that the hard excess most likely arises from Compton-scatte...
Main Authors: | Miller, L, Turner, T |
---|---|
Format: | Journal article |
Language: | English |
Published: |
2013
|
Similar Items
-
Ionized Gas Outflows from the MAGNUM Survey: NGC 1365 and NGC 4945
by: Giacomo Venturi, et al.
Published: (2017-11-01) -
Exploring the Central Region of NGC 1365 in the Ultraviolet Domain
by: Kshama Sara Kurian, et al.
Published: (2024-01-01) -
Spectral variability and reverberation time delays in the Suzaku X-ray
spectrum of NGC 4051
by: Miller, L, et al.
Published: (2009) -
Radiation reaction for spinning black-hole scattering
by: Francesco Alessio, et al.
Published: (2022-09-01) -
No evidence for black hole spin powering of jets in X-ray binaries
by: Fender, R, et al.
Published: (2010)