Results 101 to 110 of about 64,814 (288)

The dust masses of powerful radio galaxies: clues to the triggering of their activity [PDF]

open access: yes, 2014
We use deep Herschel Space Observatory observations of a 90% complete sample of 32 intermediate-redshift 2Jy radio galaxies (0.05 < z < 0.7) to estimate the dust masses of their host galaxies and thereby investigate the triggering mechanisms for their ...
Almeida, C.   +7 more
core   +3 more sources

AGN-host connection at 0.5 [PDF]

open access: yes, 2016
We explore the dependence of the incidence of moderate-luminosity (L 0.5−8 keV = 1041.9−43.7 erg s-1 ) active galactic nuclei (AGNs) and the distribution of their accretion rates on host color at 0.5 ∗ > 1010 M ⊙ .
Tao Wang   +18 more
semanticscholar   +1 more source

Comparing the host galaxy ages of X-ray selected AGN in COSMOS

open access: yesAstronomy & Astrophysics, 2023
We explore the properties of the host galaxies of X-ray selected AGN in the COSMOS field using the Chandra Legacy sample and the LEGA-C survey VLT optical spectra. Our main goal is to compare the relative ages of the host galaxies of the obscured and unobscured AGN by means of the calcium break Dn(4000) and the Hδ Balmer line.
Georgantopoulos, I.   +5 more
openaire   +4 more sources

Star-formation in the host galaxies of radio-AGN [PDF]

open access: yesProceedings of Nuclei of Seyfert galaxies and QSOs - Central engine & conditions of star formation — PoS(Seyfert 2012), 2013
There exist strong evidence supporting the co-evolution of central supermassive black holes and their host galaxies. It is however still unclear what the exact role of nuclear activity, in the form of accretion onto these supermassive black holes, in this co-evolution is.
Karouzos, Marios   +4 more
openaire   +4 more sources

Morphologies of Radio, X-Ray, and Mid-Infrared Selected AGN

open access: yes, 2010
We investigate the optical morphologies of candidate active galaxies identified at radio, X-ray, and mid-infrared wavelengths. We use the Advanced Camera for Surveys General Catalog (ACS-GC) to identify 372, 1360, and 1238 AGN host galaxies from the VLA,
Alonso-Herrero   +46 more
core   +1 more source

The black holes of radio galaxies during the "Quasar Era": Masses, accretion rates, and evolutionary stage [PDF]

open access: yes, 2010
We present an analysis of the AGN broad-line regions of 6 powerful radio galaxies at z>~2 (HzRGs) with rest-frame optical imaging spectroscopy obtained at the VLT. All galaxies have luminous (L(H-alpha)=few x 10^44 erg s^-1), spatially unresolved H-alpha
Best, Philip N.   +5 more
core   +1 more source

Star-forming Nuclear Clusters in Dwarf Galaxies Mimicking Active Galactic Nucleus Signatures in the Mid-infrared

open access: yesThe Astrophysical Journal
Effectively finding and identifying active galactic nuclei (AGNs) in dwarf galaxies is an important step in studying black hole formation and evolution.
Megan R. Sturm   +2 more
doaj   +1 more source

Properties of Galaxies Hosting X-ray Selected Active Galactic Nuclei in the Cl1604 Supercluster at z=0.9 [PDF]

open access: yes, 2008
To investigate the role of feedback from Active Galactic Nuclei (AGN) in driving the evolution of their host galaxies, we have carried out a study of the environments and optical properties of galaxies harboring X-ray luminous AGN in the Cl1604 ...
Abraham   +71 more
core   +2 more sources

The abundances and properties of Dual AGN and their host galaxies in the EAGLE simulations [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
We look into the abundance of Dual AGN (active galactic nucleus) in the largest hydrodynamical simulation from the Evolution and Assembly of GaLaxies and their Environment (EAGLE) project.
Y. Rosas-Guevara   +4 more
semanticscholar   +1 more source

Study of AGN contribution on morphological parameters of their host galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2019
AbstractWe tested how the AGN contribution (5%–75% of the total flux) may affect different morphological parameters commonly used in galaxy classification. We carried out all analysis at z ∼ 0 and at higher redshifts that correspond to the COSMOS field.
Getachew-Woreta, Tilahun   +5 more
openaire   +5 more sources

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