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We report on an identification of a new gamma-ray emitting narrow-line Seyfert 1 galaxy (gamma-NLS1), SDSS J095909.51+460014.3 (z = 0.399), by establishing an association with a gamma-ray source 4FGL 0959.6+4606, although its low-energy…

高能天体物理现象 · 物理学 2023-07-26 Yang-Ji Li , Neng-Hui Liao , Zhen-feng Sheng , Sina Chen , Yi-Bo Wang , Ting-Gui Wang

Narrow-line Seyfert 1 (NLSy1) galaxies are an enigmatic class of active galactic nuclei (AGN) that exhibit peculiar multiwavelength properties across the electromagnetic spectrum. For example, these sources have allowed us to explore the…

星系天体物理 · 物理学 2023-11-27 Vaidehi S. Paliya , C. S. Stalin , Alberto Dominguez , D. J. Saikia

We probed the relation between properties of Seyfert nuclei and morphology of their host galaxies. We selected Seyfert galaxies from the Sloan Digital Sky Survey with redshifts less 0.2 identified by the V\'{e}ron Catalog (13th). We used…

星系天体物理 · 物理学 2017-12-20 Yen-Chen Chen , Chorng-Yuan Hwang

ACO 3627 is a rich, nearby cluster of galaxies at the core of the Great Attractor. At the low galactic latitude of b = -7.2 the galactic extinction is significant. Nevertheless, its proximity makes it a prime target for studies of…

天体物理学 · 物理学 2007-05-23 P. A. Woudt , R. C. Kraan-Korteweg , A. P. Fairall , H. Bohringer , V. Cayatte , I. S. Glass

The jet activity of Active Galactic Nuclei (AGN), and its interaction with the interstellar medium (ISM), may play a pivotal role in the processes which regulate the growth and star formation of its host galaxy. Observational evidence which…

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…

天体物理学 · 物理学 2009-11-11 G. C. Dewangan , R. E. Griffiths

We present radio observations of the radio galaxy PKS 2152-699 obtained with the Australia Telescope Compact Array (ATCA). The much higher resolution and s/n of the new radio maps reveals the presence of a bright radio component about 10…

天体物理学 · 物理学 2009-10-30 R. A. E. Fosbury , R. Morganti , W. Wilson , R. D. Ekers , S. di Serego Alighieri , C. N. Tadhunter

The recent detection of high-energy gamma rays from Narrow-Line Seyfert 1 Galaxies has confirmed that also this type of active galactic nuclei can generate powerful relativistic jets. I outline the evolution of the knowledge in this…

高能天体物理现象 · 物理学 2013-01-25 Luigi Foschini

We report Fermi-LAT observations of the radio-loud AGN SBS 0846+513 (z=0.5835), optically classified as a Narrow-Line Seyfert 1 galaxy, together with new and archival radio-to-X-ray data. The source was not active at gamma-ray energies…

An increasing number of observations and simulations suggests that low-power (<10$^{44}$ erg s$^{-1}$) jets may be a significant channel of feedback produced by active galactic nuclei (AGN), but little is known about their actual effect on…

We present a spectroscopic and imaging study of an abnormal active galactic nucleus (AGN), 2MASX J00423991+3017515. This AGN is newly identified in the hard X-rays by the Swift BAT All-Sky survey and found in an edge-on disk galaxy…

星系天体物理 · 物理学 2021-03-17 J. Drew Hogg , Laura Blecha , Christopher S. Reynolds , Krista Lynne Smith , Lisa M. Winter

Narrow-line Seyfert 1 (NLS1) galaxies are a type of active galactic nuclei (AGN) that were originally classified as sources with little to no radio emission. Although the class is rather unified from an optical perspective, their radio…

星系天体物理 · 物理学 2025-11-26 I. Varglund , E. Järvelä , M. J. Hardcastle , S. Varglund , A. Lähteenmäki

We study a sample of Narrow-line Seyfert 1 galaxies (NLS1) in their optical and radio features, in order to understand the differences between their radio silent, radio-loud and radio-quiet subclasses. We first show that the different…

星系天体物理 · 物理学 2018-08-15 Tullia Sbarrato , Massimo Dotti , Giancarlo Ghirlanda , Fabrizio Tavecchio

Extended narrow-line regions (ENLRs) and extended emission-line regions (EELRs) have been the focus of integral field spectroscopy aiming at the inner kiloparsecs of nearby Seyfert galaxies as well as the larger environment of high redshift…

宇宙学与河外天体物理 · 物理学 2011-07-05 J. Scharwaechter , M. A. Dopita , J. Zuther , S. Fischer , S. Komossa , A. Eckart

Flat-spectrum radio-loud Narrow-Line Seyfert 1 galaxies (NLS1s) are a recently discovered class of $\gamma$-ray emitting Active Galactic Nuclei (AGN), that exhibit some blazar-like properties which are explained with the presence of a…

In Paper I, we exploited the unsurpassed resolution and depth of JWST/NIRCam imagery to investigate the relationship between AGN and host-galaxy properties in the JWST era, finding a correlation between the level of spatial disturbance (as…

The unified model of active galactic nuclei (AGN) predicts silicate emission features at 10 and 18 microns in type 1 AGN, and such features have now been observed in objects ranging from distant QSOs to nearby LINERs. More surprising,…

星系天体物理 · 物理学 2009-11-13 R. E. Mason , N. A. Levenson , Y. Shi , C. Packham , V. Gorjian , K. Cleary , J. Rhee , M. Werner

$\gamma$-ray-emitting narrow-line Seyfert 1 galaxies ($\gamma$-NLS1) constitute an intriguing small population of Active Galactic Nuclei with $\gamma$-ray emission resembling low power flat-spectrum radio quasars (FSRQ), but with differing…

高能天体物理现象 · 物理学 2023-05-31 Anna Luashvili , Catherine Boisson , Andreas Zech , Maialen Arrieta-Lobo , Daniel Kynoch

(Abridged) We describe a sample of low-mass Seyfert 2 galaxies selected from the Sloan Digital Sky Survey, having a median absolute magnitude of M_g = -19.0 mag. These galaxies are Type 2 counterparts to the Seyfert 1 galaxies with…

天体物理学 · 物理学 2009-11-13 A. J. Barth , J. E. Greene , L. C. Ho

The discovery of the M-sigma relation, the local galaxy bimodality, and the link between black-hole and host-galaxy properties, have raised the question whether AGN play a role in galaxy evolution. Several theoretical models implement AGN…

星系天体物理 · 物理学 2014-12-24 M. Vitale , L. Fuhrmann , M. Garcia-Marin , A. Eckart , J. Zuther , A. M. Hopkins