Astrophysics (Index)About

Compton reflection

(recognizable emission due to a gas or plasma's Compton scattering)

The term Compton reflection is used for a spectral signature observed in EMR from active galactic nuclei (AGNs), indicating a spectrum resulting from Compton scattering of photons from a power-law X-ray source (decreasing with frequency). The term Compton reflection is used for the resulting spectral feature, a characteristic "hump" (Compton hump) in the observed spectral energy distribution (SED), but the term is also sometimes taken to include emission lines indicating fluorescence of particular elements.

Such power-law spectra (in the X-ray spectral band) generated within AGNs are inferred from their explaining power regarding the observed SED. The Compton reflection is presumed to be generated in a cooler gas cloud near (e.g., immediately in front of) the AGN's internal X-ray source. The presence of iron lines that imply absorption of high-energy photons provide more evidence for the model.

Models have been developed regarding mechanisms by which the AGN's black-hole accretion could generate such a power-law spectrum.


(EMR,AGN,X-ray,spectral feature)
Further reading:
https://ui.adsabs.harvard.edu/abs/1999ASPC..161..178R/abstract
http://www.isdc.unige.ch/~ricci/Website/AGN_in_the_X-ray_band.html
https://ui.adsabs.harvard.edu/abs/1991MNRAS.249..352G/abstract

Referenced by pages:
AGN corona
corona
K-line
spectral feature

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