Results 41 to 50 of about 152,801 (176)
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
AGN Obscuration and the Unified Model
Unification Models of Active Galactic Nuclei postulate that all the observed differences between type 1 and type 2 objects are due to orientation effects with respect to the line of sight to the observer. The key ingredient of these models is the obscuring medium, historically envisaged as a toroidal structure on a parsec scale.
Stefano Bianchi +3 more
wiley +1 more source
A Practical Guide to the Massive Black Hole Cosmic History
I review our current understanding of massive black hole (MBH) formation and evolution along the cosmic history. After a brief introductory overview of the relevance of MBHs in the hierarchical structure formation paradigm, I discuss the main viable channels for seed BH formation at high redshift and for their subsequent mass growth and spin evolution.
A. Sesana, Francesco Shankar
wiley +1 more source
We analyze a sample of ~113,000 galaxies ( z
Huynh Anh N. Le, Yongquan Xue
doaj +1 more source
Of the 271 sources in the 3rd EGRET catalogue, 131 were reported as unidentied, i.e. not associated with any particular class of point source in the sky.
Pieter J. Meintjes +3 more
doaj +1 more source
A Comparison of Star Formation Rates by Different Tracers in Nearby Galaxies
We utilize a large sample of ∼113,000 galaxies ( z < 0.3) from the Sloan Digital Sky Survey with high-quality data to compare star formation rates (SFRs) across multiple diagnostic methods and examine their connection to the strength of active galactic ...
Huynh Anh N. Le +5 more
doaj +1 more source
Large scale environments of narrow-line Seyfert 1 galaxies
Narrow lines Seyfert galaxies and their ...
Lietzen Heidi (5293012) +4 more
core +1 more source
Continuous Filament Network of the Local Universe
Simulated galaxy distributions are suitable for developing filament detection algorithms. However, samples of observed galaxies, being of limited size, cause difficulties that lead to a discontinuous distribution of filaments.
Anatoliy Tugay, Mariusz Tarnopolski
doaj +1 more source
Star formation in Seyfert galaxies [PDF]
An analysis of the IRAS data for a sample of classical (optically selected) Seyfert galaxies is presented. The IRAS fluxes at 25 micron, 60 micron, and 100 micron are found to be uncorrelated or only very weakly correlated with the UV/Optical continuum ...
Espinosa, J. M. Rodriguez +2 more
core
REGARDING THE POSSIBLE WAYS OF EVOLUTION OF SEYFERT GALAXIES [PDF]
Changes of some physical parameters obtained from the theoretical model calculations in several catalogs for Seyfert galaxies of spectral classes Sy 1 and Sy 2 are analyzed in the present work and a conclusion suggesting that there is a high probability ...
Khalilov, V.M. +2 more
core

