Results 41 to 50 of about 132,127 (94)

Large-Scale Environment Properties of Narrow-Line Seyfert 1 Galaxies at z < 0.4

open access: yesFrontiers in Astronomy and Space Sciences, 2017
The large-scale environment is believed to affect the evolution and intrinsic properties of galaxies. It offers a new perspective on narrow-line Seyfert 1 galaxies (NLS1) which have not been extensively studied in this context before.
Emilia Järvelä   +5 more
doaj   +1 more source

Forty Years of X-Raying Narrow-Line Seyfert 1 Galaxies

open access: yesActa Polytechnica CTU Proceedings, 2014
Forty years after the discovery of Narrow-Line Seyfert 1 Galaxies (NLS1s), and 20 years since the discovery of the remarkable ultrasoft soft X-ray emissions of NLS1s, strategic publications improved the understanding of the Seyfert phenomenon more ...
Thomas Boller
doaj   +1 more source

Stellar and dust properties in a sample of blue early type galaxies [PDF]

open access: yesSerbian Astronomical Journal, 2022
This paper presents a comparative study of physical properties of a sample of 89 blue early-type galaxies (ETGs) from the local universe by fitting SEDs to their multi-wavelength photometric and spectroscopic data.
Deshmukh S.P.   +2 more
doaj   +1 more source

Soft X-ray properties of a spectroscopically selected sample of interacting and isolated Seyfert galaxies [PDF]

open access: yes, 2001
We present a catalogue of ROSAT detected sources in the sample of spectroscopically selected Seyfert 1 and Seyfert 2 galaxies of Rafanelli et al. (1995). The catalogue contains 102 Seyfert 1 and 36 Seyfert 2 galaxies. The identification is based on X-ray contour maps overlaid on optical images taken from the Digitized Sky Survey.
arxiv   +1 more source

Type 2 counterparts of narrow-line Seyfert 1 galaxies [PDF]

open access: yesAstrophys.J. 625 (2005) L31-L34, 2005
Unified models of Seyfert galaxies, based on viewing angles, successfully explain the observed differences between type 1 and 2 Seyferts. The existence of a range in accretion rates relative to the Eddington rate (from broad-line Seyfert 1s to narrow-line Seyfert 1s or NLS1s) and the unification of Seyfert galaxies imply that there must be type 2 ...
arxiv   +1 more source

Modelling the Multifrequency SED of AGN Candidates among the Unidentied EGRET and Fermi Gamma-Ray Sources

open access: yesActa Polytechnica CTU Proceedings, 2014
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

Growth of Accreting Supermassive Black Hole Seeds and Neutrino Radiation

open access: yesJournal of Astrophysics, Volume 2015, Issue 1, 2015., 2015
In the framework of microscopic theory of black hole (MTBH), which explores the most important processes of rearrangement of vacuum state and spontaneous breaking of gravitation gauge symmetry at huge energies, we have undertaken a large series of numerical simulations with the goal to trace an evolution of the mass assembly history of 377 plausible ...
Gagik Ter-Kazarian, Gary Wegner
wiley   +1 more source

Retrograde versus Prograde Models of Accreting Black Holes

open access: yesAdvances in Astronomy, Volume 2013, Issue 1, 2013., 2013
There is a general consensus that magnetic fields, accretion disks, and rotating black holes are instrumental in the generation of the most powerful sources of energy in the known universe. Nonetheless, because magnetized accretion onto rotating black holes involves both the complications of nonlinear magnetohydrodynamics that currently cannot fully be
David Garofalo, Alberto J. Castro-Tirado
wiley   +1 more source

Spectra of X-ray galaxies in filaments

open access: yesВісник Астрономічної школи, 2013
Large-scale structure of Universe consists of galaxy clusters connected by filaments. Single filaments can be detected at redshifts up to 0.15. The general characteriscis of X-ray spectra of Sloan Digital Sky Survey galaxies, that lies outside clusters ...
A. V Tugay
doaj   +1 more source

Jetted Narrow-Line Seyfert 1 Galaxies & Co.: Where Do We Stand?

open access: yesUniverse, 2020
The discovery in 2008 of high-energy gamma-rays from Narrow-Line Seyfert 1 Galaxies (NLS1s) made it clear that there were active galactic nuclei (AGN) other than blazars and radio galaxies that can eject powerful relativistic jets.
Luigi Foschini
doaj   +1 more source

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