In NGC 7582, low-ionization lines trace ordered disk rotation while high-ionization lines trace the AGN outflow, with intermediate lines separated via a thin disk plus hollow-bicone model showing the outflow exceeds escape velocity.
This line strongly traces the circumnuclear star-forming disk and is well fit by a single-Gaussian plus continuum fit
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Decoupling the AGN outflow and star-forming disk kinematics in the nuclear region of NGC 7582 with JWST NIRSpec and MIRI/MRS
In NGC 7582, low-ionization lines trace ordered disk rotation while high-ionization lines trace the AGN outflow, with intermediate lines separated via a thin disk plus hollow-bicone model showing the outflow exceeds escape velocity.