The hot corona of an AGN is reinterpreted as a plasmoid chain in a parabolic reconnection layer, whose height tracks X-ray luminosity in a way that resembles IRAS 13224-3809 once a magnetic parameter is fitted.
Title resolution pending
1 Pith paper cite this work, alongside 60 external citations. Polarity classification is still indexing.
1
Pith paper citing it
60
external citations · OpenAlex
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
A New Interpretation for the Hot Corona in Active Galactic Nuclei
The hot corona of an AGN is reinterpreted as a plasmoid chain in a parabolic reconnection layer, whose height tracks X-ray luminosity in a way that resembles IRAS 13224-3809 once a magnetic parameter is fitted.