A unified topology-based explanation of broadened line profile morphology from equatorial accretion disks, with a classification of all shapes under the standard thin-disk model and a demonstration that these shapes are sensitive to deviations from Keplerian motion.
Cunningham prescribes that particles interior to the ISCO travel on geodesics while maintaining the conserved quantities as- sociated with an ISCO orbiter [29]
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Morphology of Relativistically Broadened Line Emission from Axisymmetric Equatorial Accretion Disks
A unified topology-based explanation of broadened line profile morphology from equatorial accretion disks, with a classification of all shapes under the standard thin-disk model and a demonstration that these shapes are sensitive to deviations from Keplerian motion.