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"A significantly stronger reflection in a certain class of AGN indicates that the environment of these objects is different," comments co-author Roland Walter, who is the Principal Investigator of the INTEGRAL team at the ISDC. "The discrepancy in the high-energy emission properties of different AGN types is unaccounted for in the leading theoretical framework and calls for a rethinking of some of its details," he adds.
In the light of the new data, the unified model's basic assumption that the same central engine powers all AGN is safe. However, the presumed existence, in all of them, of an anisotropic, toroidal structure needs revision. "We argue that various classes of AGN are characterised by a substantially different distribution of absorbing material around the black hole," notes Walter.
"A significantly stronger reflection in a certain class of AGN indicates that the environment of these objects is different," comments co-author Roland Walter, who is the Principal Investigator of the INTEGRAL team at the ISDC. "The discrepancy in the high-energy emission properties of different AGN types is unaccounted for in the leading theoretical framework and calls for a rethinking of some of its details," he adds.
The team advocate a patchy but overall isotropic morphology for the absorber. In this scenario, the density of clouds around the central source would determine the amount of reflected X-rays, with denser environments resulting in stronger reflection. The astronomers speculate about whether such morphological variations could characterise objects at different evolutionary stages, although the issue is still unclear and the subject of further investigation.
Now, the study by Ricci and his colleagues proposes a fresh solution to the puzzle: when the reflected X-rays are added to the total budget of radiation sources in the CXB, invoking sources that have never been observed may no longer be necessary.
Originally posted by TrueBrit
Right, so basicaly the punchline here, is that rather than all active galactic nuclei operating in the exact same fashion , we have a revalation which points to the possibility of certain idiosyncratic elements comming out in the observable data we recieve from researchers and thier telescopes?
From the article , it seems to me that they are suggesting that the various different reflections and levels of reflections they are observing, are leading them to the conclusion that there are differences in the way certain classes of AGN behave. But the reflectivity of the stuff around these centres of activity is , I would have thought, bound to vary slightly , as not all regions of space contain the exact same proportion of elemental ingredients. Surely if one sort of galaxy is reflecting different levels (of light?) that might mean that slightly different matter, as well as more or less matter, is being collected around the core?
Or have I completely missed the point?