Results 11 to 20 of about 64,814 (288)

The bulge-disc decomposition of AGN host galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
We present the results from a study of the morphologies of moderate luminosity X-ray selected AGN host galaxies in comparison to a carefully mass-matched control sample at 0.5 99.7% confidence level, according to all model fits even those which adopt a ...
V. Bruce   +5 more
semanticscholar   +6 more sources

The Host Galaxies of AGN [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2003
We examine the properties of the host galaxies of 22,623 narrow-line AGN with 0 ...
G. Kauffmann   +12 more
semanticscholar   +6 more sources

AGN Absorption Linked to Host Galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2013
Multiwavelength identification of AGN is crucial not only to obtain a more complete census, but also to learn about the physical state of the nuclear activity (obscuration, efficiency, etc.).
Juneau, Stéphanie
core   +3 more sources

GALAXIES ON DIET: FEEDBACK SIGNATURES IN RADIO-AGN HOST GALAXIES [PDF]

open access: bronzePublications of The Korean Astronomical Society, 2017
There exists strong evidence supporting the co-evolution of central supermassive black holes and their host galaxies; however it is still under debate how such a relation comes about and whether it is relevant for all or only a subset of galaxies. An important mechanism connecting AGN to their host galaxies is AGN feedback, potentially heating up or ...
Marios Karouzos   +21 more
openalex   +4 more sources

The mass-metallicity and fundamental metallicity relations in non-AGN and AGN-host galaxies [PDF]

open access: hybridMonthly notices of the Royal Astronomical Society
Galaxies’ stellar masses, gas-phase oxygen abundances (metallicity), and star formation rates (SFRs) obey a series of empirical correlations, most notably the mass-metallicity relation (MZR) and fundamental metallicity relation (FZR), which relates ...
Songlin Li   +7 more
openalex   +3 more sources

A Morphological Study of AGN-host Dwarf Galaxies

open access: yesThe Astrophysical Journal
The study of morphology in galaxies offers a convenient and quantitative method to measure the shapes and characteristics of galaxy light distribution that reflect the evolutionary history.
Jie Tian   +3 more
doaj   +3 more sources

Clustering, host galaxies, and evolution of AGN

open access: green, 2009
We explore the connection between different classes of active galactic nuclei (AGNs) and the evolution of their host galaxies, by deriving host galaxy properties, clustering, and Eddington ratios of AGNs selected in the radio, X-ray, and infrared (IR) wavebands from the wide-field (9 deg^2) Bootes survey.
Ryan C. Hickox
openalex   +4 more sources

The Interplay between Radio AGN Activity and Their Host Galaxies [PDF]

open access: goldGalaxies, 2023
Radio activity in AGN (Active Galactic Nuclei) produce feedback on the host galaxy via the impact of the relativistic jets on the circumnuclear gas. Although radio jets can reach up to several times the optical radius of the host galaxy, in this review we focus on the observation of the feedback deposited locally in the central region of the host ...
Guilherme S. Couto   +1 more
openalex   +4 more sources

AGN host galaxies at redshift z 0.7: peculiar or not? [PDF]

open access: yesAstronomy & Astrophysics, 2012
Aims. We perform a quantitative morphological comparison between the hosts of active galactic nuclei (AGN) and quiescent galaxies at intermediate redshifts (z ≈ 0.7).
A. Boehm   +23 more
semanticscholar   +8 more sources

HERSCHEL OBSERVED STRIPE 82 QUASARS AND THEIR HOST GALAXIES: CONNECTIONS BETWEEN AGN ACTIVITY AND HOST GALAXY STAR FORMATION [PDF]

open access: green, 2016
In this work, we present a study of 207 quasars selected from the Sloan Digital Sky Survey quasar catalogs and the Herschel Stripe 82 survey. Quasars within this sample are high-luminosity quasars with a mean bolometric luminosity of 1046.4 erg s−1.
Xiaoyi Dong, Xue-Bing Wu
openalex   +3 more sources

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