A z=6.64 LRD host galaxy exhibits a fast AGN-driven outflow with 5500 km/s velocities, dusty gas, and low metallicity, confirming AGN presence in these systems.
Theoretical values for the [O iii] 5007/4959 line-intensity ratio and homologous cases
2 Pith papers cite this work, alongside 542 external citations. Polarity classification is still indexing.
2
Pith papers citing it
542
external citations · external index
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A homogeneous analysis of 699 spectra yields Te-Te relations for ions including N II, O II, O III, S II, S III and Ar III, with lower dispersions for relations involving Te([N II]).
citing papers explorer
-
GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy
A z=6.64 LRD host galaxy exhibits a fast AGN-driven outflow with 5500 km/s velocities, dusty gas, and low metallicity, confirming AGN presence in these systems.
-
The DESIRED electron temperature relations in star-forming regions of the local Universe
A homogeneous analysis of 699 spectra yields Te-Te relations for ions including N II, O II, O III, S II, S III and Ar III, with lower dispersions for relations involving Te([N II]).