Results 161 to 170 of about 64,814 (288)
The Complex Multiwavelength Morphology of the Peculiar Compact Galaxy Group IC 2431
We present new Chandra X-ray imaging spectroscopy of the compact galaxy group IC 2431, and compare with archival ultraviolet, optical, infrared, and radio images. IC 2431 is a starburst system containing three tidally distorted disk galaxies.
Beverly J. Smith +5 more
doaj +1 more source
Morphologies of low-redshift AGN host galaxies: what role does AGN luminosity play?
Mergers of galaxies have been suspected to be a major trigger of AGN activity for many years. However, when compared to carefully matched control samples, AGN host galaxies often show no enhanced signs of interaction.
Chang, YuYen +9 more
core
X-Ray Bright Active Galactic Nuclei in Local Dwarf Galaxies: Insights from eROSITA
Although supermassive black holes (SMBHs) reside in the heart of virtually every massive galaxy, it remains debated whether dwarf galaxies commonly host SMBHs. Because low-mass galaxies may retain memory of the assembly history of their black holes (BHs),
Andrea Sacchi +3 more
doaj +1 more source
The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey [PDF]
Elisabeta Lusso +17 more
openalex +1 more source
We examine the demographics of radio-emitting active galactic nuclei (AGN) in the local Universe as a function of host galaxy properties, most notably both stellar mass ( M _⋆ ) and star formation rate (SFR).
Arjun Suresh, Michael R. Blanton
doaj +1 more source
Accretion history of AGN: Estimating the host galaxy properties in X-ray luminous AGN from z = 0–3 [PDF]
Brandon Coleman +12 more
openalex +1 more source
Prevalence of galaxy-galaxy interactions in AGN hosts [PDF]
Cheng-Yu Kuo +4 more
openaire +2 more sources
JWST is revolutionizing our view of the early Universe by pushing the boundaries of detectable galaxies and black holes in redshift (upward) and mass (downward).
Emmanuel Durodola +2 more
doaj +1 more source
Agn Host Galaxy Properties And Mass Function
Supermassive black hole growth, nuclear activity, and galaxy evolution have been found to be closely related. In the context of AGN-galaxy coevolution, I will discuss about the relation found between the host galaxy properties and the central BH and I will present the latest determination of the host galaxy stellar mass function (HGMF), and the ...
openaire +2 more sources
In terms of the variable nature of normal active galaxy nuclei (AGN) and luminous quasars, a so-called flux variation gradient (FVG) method has been widely utilized to estimate the underlying non-variable host galaxy fluxes.
Minxuan Cai +4 more
doaj +1 more source

