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相关论文: Evidence for Relativistic Outflows in Narrow-line …

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We present \chandra high energy transmission grating spectra of the narrow-line Seyfert-1 galaxy Ark 564. The spectrum shows numerous absorption lines which are well modeled with low velocity outflow components usually observed in Seyfert…

高能天体物理现象 · 物理学 2015-06-12 A. Gupta , S. Mathur , Y. Krongold , F. Nicastro

We present evidence that the outflowing UV absorbers in Seyfert 1 galaxies arise primarily in their inner narrow (emission) line regions (NLRs), based on similarities in their locations, kinematics, and physical conditions. 1) Hubble Space…

天体物理学 · 物理学 2009-11-10 D. M. Crenshaw , S. B. Kraemer

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

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

In the HST/COS spectrum of the Seyfert 1 galaxy 2MASX J14292507+4518318, we have identified a narrow absorption line (NAL) outflow system with a velocity of -151 km s$^{-1}$ This outflow exhibits absorption troughs from the resonance states…

星系天体物理 · 物理学 2023-11-30 Maryam Dehghanian , Nahum Arav , Doyee Byun , Gwen Walker , Mayank Sharma

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

The emission and absorption attributes of the UV-blue nuclear spectra of the Narrow-Line Seyfert 1 (NLS1) galaxies are analyzed based on high quality archival HST observations. Measurements from composite spectra as well as from individual…

天体物理学 · 物理学 2007-05-23 Anca Constantin , Joseph C. Shields

There is growing evidence for the presence of blueshifted Fe K absorption lines in a number of radio-quiet AGNs and QSOs. These may be fundamental to probe flow dynamics near supermassive black holes. Here we aim at verifying and better…

Narrow-Line Seyfert 1 (NLS1) Galaxies are an important type of active galactic nucleus (AGN), generally expected to be accreting at high Eddington rate. The properties of their outflows and importance of AGN feedback remain intriguing. We…

星系天体物理 · 物理学 2023-01-18 Xiao-Dan Fu , Junfeng Wang , Xiaoyu Xu , Zhi-Xiang Zhang

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

Narrow Line Seyfert 1 (NLS1) galaxies are remarkable for their extreme continuum and emission line properties which are not well understood. New results bearing on the spectroscopic characteristics of these objects are presented here, with…

天体物理学 · 物理学 2009-11-07 Anca Constantin , Joseph C. Shields

We present MUSE observations of the field of the quasar Q0152$-$020 whose spectrum shows a Lyman limit system (LLS) at redshift $z_{\rm abs} = 0.38$, with a metallicity Z $\gtrsim 0.06$ Z$_\odot$. The low ionization metal lines associated…

We have studied the physical properties of a sample of narrow-line Seyfert 1 (NLS1) galaxies, and present a summary of our previous results, and new results. In particular, we have previously shown that (1) the locus of NLS1 galaxies on the…

宇宙学与河外天体物理 · 物理学 2011-06-27 Dawei Xu , S. Komossa

We present four radio-loud NLS1 galaxies with extreme emission-line shifts, indicating radial outflow velocities of the ionized gas of up to 2450 km/s, above the escape velocity of the host galaxies. The forbidden lines show strong…

星系天体物理 · 物理学 2018-07-30 S. Komossa , D. W. Xu , A. Y. Wagner

While a broad profile of the Fe K$\alpha$ emission line is frequently found in the X-ray spectra of typical Seyfert galaxies, the situation is unclear in the case of Narrow Line Seyfert 1 galaxies (NLS1s)---an extreme subset which are…

高能天体物理现象 · 物理学 2015-06-23 Zhu Liu , Weimin Yuan , Youjun Lu , Xin-Lin Zhou

The narrow line Seyfert 1 (NLS1) IRAS 13224-3809 is the most X-ray variable active galactic nucleus (AGN), exhibiting 0.3-10 keV flux changes of over an order of magnitude within an hour. We report on the results of the 1.5 Ms 2016…

高能天体物理现象 · 物理学 2018-08-16 M. L. Parker , W. N. Alston , D. J. K Buisson , A. C. Fabian , J. Jiang , E. Kara , A. Lohfink , C. Pinto

Winds outflowing from Active Galactic Nuclei (AGNs) may carry significant amount of mass and energy out to their host galaxies. In this paper we report the detection of a sub-relativistic outflow observed in the Narrow Line Seyfert 1 Galaxy…

We present a detailed study of 11 narrow-line Seyfert 1 galaxies (NLS1s) from the Six-degree Field Galaxy Survey (6dFGS) that both have optical and X-ray spectroscopic observations. There are five complex NLS1s (C-NLS1s) and six simple…

星系天体物理 · 物理学 2019-10-01 S. Chen , G. La Mura , M. Berton , L. Foschini , E. Congiu , F. Di Mille , S. Ciroi , E. Bottacini , J. H. Fan , A. Vietri

We revisited the spectroscopic characteristics of narrow-line Seyfert 1 galaxies (NLS1s) by analysing a homogeneous sample of 296 NLS1s at redshift between 0.028 and 0.345, extracted from the Sloan Digital Sky Survey (SDSS-DR7) public…

星系天体物理 · 物理学 2016-08-17 V. Cracco , S. Ciroi , M. Berton , F. Di Mille , L. Foschini , G. La Mura , P. Rafanelli

The analysis of hard X-ray features in XMM-Newton data of the bright Sy 1 galaxy Mrk 335 is reported here. The presence of a broad, ionised iron K alpha emission line in the spectrum, first found by Gondoin et al.(2002), is confirmed. The…

天体物理学 · 物理学 2007-05-23 A. L. Longinotti , S. Sim , K. Nandra , M. Cappi , P. O'Neill
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