AGN dust tori can form tens of millions of planetesimals from Earth to super-Jupiter masses via streaming instability, with continued growth to stellar masses through pebble and gas accretion.
J., Cantiello, M., et al.2025
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 3roles
background 1polarities
background 1representative citing papers
AGN activity in Mrk 573 enriches the surrounding gas with metals up to several times solar abundance on 100-parsec scales via outflows and jets.
Jets escaping AGN disks decelerate rapidly in the dense wind-like medium, producing a downshifted spectrum with strong synchrotron self-absorption that creates a quasi-thermal hump, yielding detectable multi-wavelength emission outshining the AGN background with short delays after GW triggers.
citing papers explorer
-
Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets
AGN dust tori can form tens of millions of planetesimals from Earth to super-Jupiter masses via streaming instability, with continued growth to stellar masses through pebble and gas accretion.
-
Active Galactic Nuclei-driven Metallicity Enrichment in the Interstellar Medium of Mrk 573
AGN activity in Mrk 573 enriches the surrounding gas with metals up to several times solar abundance on 100-parsec scales via outflows and jets.
-
Observational Properties of Nonthermal Emission from Relativistic Jets Escaping Active Galactic Nucleus Disks
Jets escaping AGN disks decelerate rapidly in the dense wind-like medium, producing a downshifted spectrum with strong synchrotron self-absorption that creates a quasi-thermal hump, yielding detectable multi-wavelength emission outshining the AGN background with short delays after GW triggers.