Results 1 to 10 of about 31,719 (264)

Star-Forming AGN Host Galaxies [PDF]

open access: yesNew Astronomy Reviews, 2001
The symbiosis of nuclear activity and star-formation in galaxies, as manifested in their spectral energy distributions (SEDs) is reviewed. Attention is drawn to an Hertzsprung-Russell diagram-equivalent for such objects, as well as to the importance of ...
Bregman   +49 more
core   +7 more sources

The host galaxy/AGN connection. Brightness profiles of early-type galaxies hosting Seyfert nuclei [PDF]

open access: greenAstronomy & Astrophysics, 2007
[ABRIDGED] We recently presented evidence of a connection between the brightness profiles of nearby early-type galaxies and the properties of the AGN they host. The radio loudness of the AGN appears to be univocally related to the host's brightness profile: radio-loud nuclei are only hosted by ``core'' galaxies while radio-quiet AGN are only found in ``
A. Capetti, B. Balmaverde
openalex   +4 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   +2 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

The Relation between AGN and Host Galaxy Properties in the JWST Era. II. The Merger-driven Evolution of Seyferts at Cosmic Noon

open access: goldThe Astrophysical Journal
In Paper I, we exploited the unsurpassed resolution and depth of JWST/NIRCam imagery to investigate the relationship between active galactic nuclei (AGN) and host-galaxy properties in the JWST era, finding a correlation between the level of spatial ...
Nina Bonaventura   +5 more
doaj   +2 more sources

Agn Host Galaxy Properties And Mass Function

open access: green, 2016
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 ...
A. Bongiorno
openalex   +3 more sources

Colors of AGN host galaxies at 0.5

open access: green, 2004
We present the results from a study of the host galaxies of 15 optically selected AGNs with 0 ...
Sf F. Sanchez   +15 more
openalex   +2 more sources

The smallest AGN host galaxies [PDF]

open access: yesNew Astronomy Reviews, 2006
We describe our efforts to study dwarf galaxies with active nuclei, whose black holes, with masses < 10^6 M_sun, provide the best current observational constraints on the mass distribution of primordial seed black holes. Although these low-mass galaxies do not necessarily contain classical bulges, Barth, Greene, & Ho (2005) show that their ...
Greene, J. E., Barth, A. J., Ho, L. C.
openaire   +2 more sources

Relation between AGN type and host galaxy properties [PDF]

open access: yesAstronomy & Astrophysics, 2021
We use 3213 active galactic nuclei (AGNs) from the XMM-XXL northern field to investigate the relation of AGN type with host galaxy properties. Applying a Bayesian method, we derive the hardness ratios, and through these the hydrogen column density (NH) for each source. We consider those with NH > 1021.5 cm−2 as absorbed sources (type 2).
Masoura, V. A.   +3 more
openaire   +3 more sources

AGN spiral galaxies in groups: effects of bars [PDF]

open access: yes, 2014
We explore properties of barred active spiral galaxies in groups selected from the SDSS-DR7, with the aim of assessing the effects of bars on AGN and the role of the high density environment.
Alonso, Sol   +2 more
core   +4 more sources

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