We present the first spatially resolved investigation of near-infrared coronal lines in dwarf galaxies hosting active galactic nuclei (AGN), using JWST/NIRSpec integral field spectroscopy.
Archana Aravindan +22 more
doaj +1 more source
Cosmology with Velocity Dispersion based Counts of Groups and the Effect of AGN Feedback on Host Galaxy Morphology [PDF]
C. Caldwell
openalex +1 more source
SDSS-IV MaNGA: The incidence of major mergers in type I and II AGN host galaxies in the DR15 sample [PDF]
H. M. Hernández-Toledo +6 more
openalex +1 more source
The link among X-ray spectral properties, AGN structure, and the host galaxy [PDF]
G. Mountrichas +7 more
openalex +1 more source
THE RELATION BETWEEN LUMINOUS AGNs AND STAR FORMATION IN THEIR HOST GALAXIES [PDF]
Lei Xu +5 more
openalex +1 more source
The Cosmic Owl: Twin Active Collisional Ring Galaxies with Starburst Merging Front at z = 1.14
Galaxy mergers play a critical role in driving galaxy evolution, especially by transforming galaxy morphology, redistributing gas around galaxies, triggering active galactic nuclei (AGN), and stimulating star formation.
Mingyu Li +14 more
doaj +1 more source
An empirical relation to estimate host galaxy stellar light from AGN spectra
Priyanka Jalan +4 more
openalex +1 more source
Fast Outflows and Luminous He ii Emission in Dwarf Galaxies with Active Galactic Nuclei (AGN)
While stellar processes are believed to be the main source of feedback in dwarf galaxies, the accumulating discoveries of active galactic nuclei (AGN) in dwarf galaxies over recent years arouse the interest to also consider AGN feedback in them.
Weizhe Liu +8 more
doaj +1 more source
Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
Aalto S +7 more
europepmc +1 more source
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source

