Results 71 to 80 of about 6,380 (236)

Gas Motion Mapping for Three Seyfert Galaxies

open access: yesOpen Astronomy, 2011
We report the preliminary results of a kinematical study of three Seyfert galaxies selected from a sample of nearby active galactic nuclei observed using 3D spectroscopy.
Smirnova A.   +3 more
doaj   +1 more source

EVN observations of Seyfert galaxies [PDF]

open access: yesProceedings of The 9th European VLBI Network Symposium on The role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting — PoS(IX EVN Symposium), 2009
In this contribution, we report on dual-frequency EVN observations of six nuclei of Seyfert galaxies imaged previously at arcsecond resolution with the VLA. These galaxies are part of a distancelimited sample of Seyferts, for which VLBI observations are available only for the brightest objects.
Marcello Giroletti, Francesca Panessa
openaire   +2 more sources

Jetted Seyfert Galaxies at z = 0: Simulating Feedback Effects on Galactic Morphology and Beyond

open access: yesThe Astrophysical Journal
We use high-resolution cosmological zoom-in simulations to model feedback from Seyfert-type supermassive black hole (SMBH) jets onto galaxies with identical dark matter (DM) halos of log M / M _⊙  ∼ 11.8. The low-mass,  ∼10 ^6 M _⊙ , seed SMBHs have been
Julianne Goddard   +2 more
doaj   +1 more source

Very high energy gamma-ray emission of NGC 1275 and 3c382 and the possible activity nature of the Seyfert Galaxies

open access: yesEPJ Web of Conferences, 2013
Galaxy NGC 1275 is the central dominant galaxy of the Perseus Cluster of Galaxies and is of Seyfert galaxy class. NGC 1275 is known as powerful X-ray and radio source.
Sinitsyna V.Y., Sinitsyna V.G.
doaj   +1 more source

New Infrared Seyfert Galaxies

open access: yes, 1998
We present optical spectra for new infrared Seyfert galaxies obtained with the 2.16m telescope at Beijing Astronomical Observatory (BAO). After wavelength and flux calibration, they are classified by the degree of nuclear activity: nine Seyfert 2 and three Seyfert 3 galaxies.
Gu, Q. -S.   +3 more
openaire   +2 more sources

Optical colour maps of Seyfert galaxies [PDF]

open access: yesAstronomy and Astrophysics Supplement Series, 1998
9 pages, 26 figures, LaTeX, uses l-aa.sty, psfig.sty. A&AS, accepted. Grayscale JPEGs included, original color figures (gif or ps format) can be obtained only by anonymous ftp from ftp://oj287.astro.utu.fi/pub ...
openaire   +2 more sources

A Systematic Search for Active Galactic Nuclei Obscuration Variability in the Chandra Archive

open access: yesThe Astrophysical Journal
The nature of the obscuring material in active galactic nuclei (AGN) can be studied by measuring changes in the line-of-sight column density, N _H,LOS , over time. This can be accomplished by monitoring AGN over long periods of time and at all timescales.
Isaiah S. Cox   +7 more
doaj   +1 more source

Revisiting the Fraction of Radio-Loud Narrow Line Seyfert 1 Galaxies with LoTSS DR1

open access: yesUniverse, 2020
Radio-Loud narrow-line Seyfert 1 galaxies (NLS1s), especially the extremely radio-loud ones, are widely accepted as the jetted versions of NLS1s. We explore the radio-loud fraction for NLS1s with recently released LoTSS DR1 at 150 MHz.
Xu-Liang Fan
doaj   +1 more source

IceCube Search for Neutrino Emission from X-Ray Bright Seyfert Galaxies

open access: yesThe Astrophysical Journal
The recent IceCube detection of TeV neutrino emission from the nearby active galaxy NGC 1068 suggests that active galactic nuclei (AGNs) could make a sizable contribution to the diffuse flux of astrophysical neutrinos. The absence of TeV γ -rays from NGC
R. Abbasi   +424 more
doaj   +1 more source

Two Epochs of VLBI Observations of Eight KISSR Seyfert and LINER Galaxies: Suggestions of Fast and Filamentary Outflows

open access: yesThe Astrophysical Journal
We present here the results from a second epoch of phase-referenced VLBA observations of eight Seyfert and LINER galaxies from the KISSR sample. These sources were chosen based on the presence of double peaks or asymmetries in their emission lines as ...
Preeti Kharb   +6 more
doaj   +1 more source

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