X-ray timing and spectral analysis of ASKAP J174508.9-505149 detects matching periodicity and features consistent with an accreting magnetic CV.
Super-Eddington black hole accretion: Polish doughnuts and slim disks
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
The theory of highly super-Eddington black hole accretion was developed in the 1980s in Warsaw by Paczynski and his collaborators in terms of "Polish doughnuts", i.e. low viscosity, rotating accretion flows that are optically thick, radiation pressure supported, cooled by advection, and radiatively very inefficient. Polish doughnuts resemble fat tori with two narrow funnels along rotation axis. The funnels collimate radiation into beams with highly super-Eddington luminosities. "Slim disks" introduced later by Abramowicz, Lasota and collaborators, have only moderately super-Eddington accretion rates, rather disk-like shapes, and almost thermal spectra.
years
2026 2verdicts
UNVERDICTED 2representative citing papers
The E1/MS framework flags super-Eddington candidates in jetted gamma-ray AGN, with some showing jet-consistent radio properties and gamma-ray NLS1s showing xA spectra.
citing papers explorer
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The X-ray emission of the long-period transient and accreting cataclysmic variable ASKAP J174508.9-505149
X-ray timing and spectral analysis of ASKAP J174508.9-505149 detects matching periodicity and features consistent with an accreting magnetic CV.
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Flagging Super-Eddington Candidates among Jetted, {\gamma}-Ray-Emitting AGN
The E1/MS framework flags super-Eddington candidates in jetted gamma-ray AGN, with some showing jet-consistent radio properties and gamma-ray NLS1s showing xA spectra.