Results 31 to 40 of about 31,213 (262)
The gamma‐ray emission from young radio galaxies and quasars
Abstract According to radiative models, radio galaxies are predicted to produce γ‐rays from the earliest stages of their evolution onwards. The study of the high‐energy emission from young radio sources is crucial for providing information on the most energetic processes associated with these sources, the actual region responsible for this emission, as
Giacomo Principe +5 more
wiley +1 more source
Morphologies of z~0.7 AGN host galaxies in CANDELS : no trend of merger incidence with AGN luminosity [PDF]
PS would like to acknowledge funding through grant ASI I/005/11/0. DKoo would like to acknowledge funding through grant NSF AST-0808133. SJ acknowledges financial support from the EC through an ERC grant StG-257720.The processes that trigger active ...
Bell, E.~F. +26 more
core +4 more sources
Jet propagation through inhomogeneous media and shock ionization
Abstract In this contribution, we present the first numerical simulations of a relativistic outflow propagating through the inner hundreds of parsecs of its host galaxy, including atomic and ionized hydrogen, and the cooling effects of ionization. Our results are preliminary, but we observe efficient shock ionization of atomic hydrogen in interstellar ...
Manel Perucho +3 more
wiley +1 more source
The host galaxy/AGN connection [PDF]
[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 ``
Capetti, Alessandro, Balmaverde, Barbara
openaire +2 more sources
Abstract We present a detailed study of the galaxy cluster Abell 795 and of its central Fanaroff‐Riley Type 0 (FR0) radio galaxy. From an archival Chandra observation, we found a dynamically disturbed environment with evidences for sloshing of the intracluster medium.
Francesco Ubertosi +4 more
wiley +1 more source
The bulge-disc decomposition of AGN host galaxies [PDF]
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 < z < 3 in the CANDELS GOODS-S field. We apply a multi-wavelength morphological decomposition analysis to these two samples and report on the differences between the ...
V. A. Bruce +5 more
openaire +3 more sources
The Kiloparsec-scale Influence of the AGN in NGC 1068 with SALT RSS Fabry–Pérot Spectroscopy
We present Fabry–Pérot (FP) imaging and longslit spectroscopy of the nearby Seyfert II galaxy NGC 1068 using the Robert Stobie Spectrograph (RSS) on the Southern African Large Telescope (SALT) to observe the impact of the central active galactic nucleus (
Raphael E. Hviding +4 more
doaj +1 more source
Do Moderate-Luminosity Active Galactic Nuclei Suppress Star Formation? [PDF]
The growth of supermassive black holes and their host galaxies are thought to be linked, but the precise nature of this symbiotic relationship is still poorly understood. Both observations and simulations of galaxy formation suggest that the energy input
Adelman-McCarthy +36 more
core +4 more sources
AGN host galaxy mass function in COSMOS [PDF]
15 pages, 10 figures, accepted for publication in A& ...
Bongiorno, A +13 more
openaire +4 more sources
Relation between AGN type and host galaxy properties [PDF]
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

