Results 11 to 20 of about 126,286 (222)

High Redshift Quasars, Emission Lines and ‘Cloudy’

open access: yesOpen Astronomy, 2011
I describe some of the outstanding “big picture” questions in quasar research and how the development of the plasma simulation code Cloudy is being guided to answer them.
Ferland Gary J.
doaj   +1 more source

Development of Resveratrol-Loaded Herbal Extract-Based Nanocomposites and Their Application to the Therapy of Ovarian Cancer

open access: yesNanomaterials, 2018
Resveratrol (RSV) and the ethanol extract of Angelica gigas Nakai (AGN Ex)-based nanoparticles (NPs) were prepared using the nanocrystal concept. AGN/RSV NPs with 224 nm hydrodynamic size, unimodal size distribution, and negative zeta potential values ...
Suyeong Nam   +3 more
doaj   +1 more source

The cosmic evolution of radio-AGN feedback to z=1 [PDF]

open access: yes, 2014
This paper presents the first measurement of the radio luminosity function of 'jet-mode' (radiatively-inefficient) radio-AGN out to z=1, in order to investigate the cosmic evolution of radio-AGN feedback.
Best, P. N.   +4 more
core   +1 more source

The starburst-AGN connection: the role of stellar clusters in AGNs [PDF]

open access: yesAstrophysics and Space Science, 2008
Nuclear stellar clusters are a common phenomenon in spirals and in starbursts galaxies, and they may be a natural consequence of the star formation processes in the central regions of galaxies. HST UV imaging of a few Seyfert 2 galaxies have resolved nuclear starbursts in Seyfert 2 revealing stellar clusters as the main building blocks of the extended ...
Delgado, R. M. González   +4 more
openaire   +2 more sources

Microlensing-Based Studies of the Unresolved Structure of AGNs and the Composition of Lensing Galaxies

open access: yesOpen Astronomy, 2011
Multiple images of quasars formed by gravitational lensing are typically seen through the lensing galaxy. The granulation of the galaxy in stars or other compact objects induces local (‘microscopic’) but strong fluctuations in the gravitational potential
Gradolph Teresa Mediavilla   +2 more
doaj   +1 more source

Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies [PDF]

open access: yes, 2010
We present a statistical analysis of the mid-infrared (MIR) spectra of 248 luminous infrared (IR) galaxies (LIRGs) which comprise the Great Observatories All-sky LIRG Survey (GOALS) observed with the Infrared Spectrograph (IRS) on-board the Spitzer Space
Appleton, P.   +24 more
core   +3 more sources

Multiband Study of Radio Sources of the RCR Catalogue with Virtual Observatory Tools

open access: yesOpen Astronomy, 2012
We present early results of our multiband study of the RATAN Cold Revised (RCR) catalogue obtained from seven cycles of the “Cold” survey carried with the RATAN-600 radio telescope at 7.6 cm in 1980-1999, at the declination of the SS 433 source.
Zhelenkova O. P.   +3 more
doaj   +1 more source

Emission-line Diagnostics of Low Metallicity AGN [PDF]

open access: yes, 2006
Current emission-line based estimates of the metallicity of active galactic nuclei (AGN) at both high and low redshifts indicate that AGN have predominantly solar to supersolar metallicities. This leads to the question: do low metallicity AGN exist?
Groves, Brent   +2 more
core   +3 more sources

On the Heating of AGN Magnetospheres [PDF]

open access: yesUniverse, 2021
The Langmuir–Landau-Centrifugal Drive (LLCD), which can effectively “convert” gravitational energy into particles, is explored as a driving mechanism responsible for the extreme thermal luminosity acquired by some active galactic nuclei (AGN). For this purpose, we consider equations governing the process of heating of AGN magnetospheres. In particular,
Zaza Osmanov, Swadesh Mahajan
openaire   +3 more sources

FUELING THE AGN [PDF]

open access: yes, 2001
Active Galactic Nuclei are fueled from material (gas or stars) that are in general far away from the gravitational influence of the central black hole, the engine thought to be responsible for their activity. The required material has a lot of angular momentum, that is a priori quite difficult to evacuate. The various dynamical mechanisms that may play
openaire   +2 more sources

Home - About - Disclaimer - Privacy