Extended CIII] emission offset from the stars in a z=14.18 galaxy indicates outflows with mass outflow rate ~160 solar masses per year and mass-loading factor 4-15, constraining star-formation efficiency to below 0.08.
Title resolution pending
5 Pith papers cite this work. Polarity classification is still indexing.
years
2026 5representative citing papers
A QPO candidate in NGC 1566 supports misaligned accretion flows fueled by captured broad-line region clouds as the cause of rapid changing-look AGN transitions.
Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.
citing papers explorer
-
Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0
Extended CIII] emission offset from the stars in a z=14.18 galaxy indicates outflows with mass outflow rate ~160 solar masses per year and mass-loading factor 4-15, constraining star-formation efficiency to below 0.08.
-
X-ray Quasi-Periodic Oscillations in Active Galactic Nuclei and Their Implications for the Changing Look Phenomenon
A QPO candidate in NGC 1566 supports misaligned accretion flows fueled by captured broad-line region clouds as the cause of rapid changing-look AGN transitions.
-
Very High Energy Gamma Rays from Ultra Fast Outflows
Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.
-
Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.
-
Source identification for the Swift-BAT 150-month hard X-ray catalog using soft X-ray observations
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.