The hard X-ray spectrum of NGC 1365: scattered light, not black hole
spin

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...

Deskribapen osoa

Xehetasun bibliografikoak
Egile Nagusiak:	Miller, L, Turner, T
Formatua:	Journal article
Hizkuntza:	English
Argitaratua:	2013

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