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相关论文: Narrow-Line Seyfert 1s: 15 Years Later

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The number of publications considering Narrow-Line Seyfert 1 galaxies has increased dramatically in recent years. Especially after the launch of the X-ray missions ROSAT and ASCA, Narrow-Line Seyfert 1s have become very popular. In these…

天体物理学 · 物理学 2009-10-31 Dirk Grupe

Narrow-line Seyfert 1 galaxies, with their extreme properties, defy our current knowledge of active galactic nuclei and relativistic jet systems. They excite, and might help us answer, many questions concerning the evolution and unification…

星系天体物理 · 物理学 2016-03-15 Emilia Järvelä , Anne Lähteenmäki

Narrow Line Seyfert 1 galaxies represent a distinct category in the larger family of Type 1 Active Galactic Nuclei. The occurrence of emission line profiles not broader than 2000 km/s, combined with luminosity estimates comparable to those…

高能天体物理现象 · 物理学 2011-06-14 G. La Mura , S. Ciroi , V. Cracco , D. Ilić , L. Č. Popović , P. Rafanelli

Narrow Line Seyfert 1 galaxies (NLS1) are very interesting objects which display peculiar properties when compared to their broad line analogues (BLS1). Although well studied in many wavebands, their behaviour at >10 keV is poorly studied…

天体物理学 · 物理学 2009-11-13 A. Malizia , L. Bassani , A. J. Bird , R. Landi , N. Masetti , A. De Rosa , F. Panessa , M. Molina , A. J. Dean , M. Perri , J. Tueller

No. Due to their apparently extreme optical to X-ray properties, Narrow Line Seyfert 1s (NLSy1s) have been considered a special class of active galactic nuclei (AGN). Here, we summarize observational results from different groups to…

[Abridged] Narrow-line Seyfert 1 (NLS1) galaxies are a class of active galactic nuclei (AGN) that have all the properties of type 1 Seyfert galaxies but show peculiar characteristics, including the narrowest Balmer lines, strongest Fe II…

宇宙学与河外天体物理 · 物理学 2015-05-28 A. Tarchi , P. Castangia , A. Columbano , F. Panessa , J. A. Braatz

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. In…

高能天体物理现象 · 物理学 2020-09-01 Luigi Foschini

We have discovered a Narrow-Line Seyfert 1 (NLS1) galaxy and identified it with an ultrasoft X-ray source RX 215319-1514 detected with ROSAT. We present its X-ray and optical spectral characteristics. Its redshift is found to be…

天体物理学 · 物理学 2007-05-23 K. P. Singh , L. R. Jones

We describe how recent X-ray surveys have led to advances in the understanding of ultrasoft narrow-line Seyfert 1 galaxies. The number of known ultrasoft narrow-line Seyfert 1s has increased greatly in recent years due to X-ray surveys, and…

天体物理学 · 物理学 2009-09-25 W. N. Brandt , Th. Boller

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

I provide a short review of the properties of Narrow-line Seyfert 1 (NLS1) galaxies across the electromagnetic spectrum and of the models to explain them. Their continuum and emission-line properties manifest one extreme form of Seyfert…

天体物理学 · 物理学 2007-10-18 S. Komossa

Thanks to the execution of extensive spectroscopic surveys that have covered large fractions of the sky down to magnitudes as faint as $i \approx 19$, it has been possible to identify several narrow-line Seyfert 1 galaxies (NLS1s) and to…

星系天体物理 · 物理学 2018-09-10 G. La Mura , D. Bastieri , M. Berton , S. Chen , S. Ciroi , E. Congiu , V. Cracco , J. -H. Fan , P. Rafanelli

Narrow-line Seyfert\,1 galaxies (NLS1s) with very small broad-line widths (say, FWHM(\hb) $\la $ 1200\,\kms) represent the extreme type of Seyfert\,1 galaxies that have small black hole masses (\mbh) and/or high Eddington ratios (\redd).…

高能天体物理现象 · 物理学 2015-05-20 Y. L. Ai , W. Yuan , H. Y. Zhou , T. G. Wang , S. H. Zhang

Narrow Line Seyfert 1 galaxies (NLS1s) are intriguing due to their continuum as well as emission line properties. The observed peculiar properties of the NLS1s are believed to be due to accretion rate close to Eddington limit. As a…

天体物理学 · 物理学 2016-08-30 Smita Mathur

X-ray spectral features which are unusually strong in many Narrow-Line Seyfert galaxies are found to be consistent with reflection from strongly ionized matter, providing further evidence of a high accretion rate in these objects and…

天体物理学 · 物理学 2009-10-31 K. Pounds , S. Vaughan

We report on AGN with extremely soft X-ray spectra observed with ROSAT. From their optical emission lines these objects are classified as narrow-line Seyfert 1 galaxies (NLS1), almost all with extremely large Fe II/H-beta ratios and…

天体物理学 · 物理学 2007-05-23 Th. Boller , W. N. Brandt , H. Fink

We have compiled a list of 83 objects classified as Narrow-Line Seyfert 1 galaxies (NLS1s) or known to have a broad Balmer component narrower than 2000 km/s. Out of these, 19 turned out to have been spectroscopically misidentified in…

天体物理学 · 物理学 2009-11-06 M. -P. Veron-Cetty , P. Veron , A. C. Goncalves

We report the discovery of gamma-ray emission from two radio-loud narrow-line Seyfert 1 galaxies using data from Fermi/LAT: J0804+3853 (z = 0.211) and J1443+4725 (z = 0.502). The objects were discovered due to singular, separate, and brief…

高能天体物理现象 · 物理学 2014-04-29 Joseph R. Eggen , Jeremy D. Maune , H. R. Miller

The recent observations of highly accreting supermassive black holes (SMBH) at very high redshift ($>$4) with the James Webb Space Telescope (JWST) allowed us to shed light for the very first time on the early evolutionary phases of active…

星系天体物理 · 物理学 2025-09-05 M. Berton , E. Järvelä , A. Tortosa , C. Mazzucchelli

Narrow-Line Seyfert 1s (NLS1s) are generally considered to be strange Active Galactic Nuclei (AGNs). Surprisingly, this makes them very useful for constraining models. I discuss what happens when one attempts to qualitatively fit the NLS1…

天体物理学 · 物理学 2009-10-31 Jason A. Taylor
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