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相关论文: Narrow Line Seyfert 1 galaxies at hard X-rays

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We report the analysis of all Swift observations available up to 2019 April of $\gamma$-ray-emitting narrow-line Seyfert 1 galaxies (NLSy1). The distribution of X-ray luminosities (and fluxes) indicates that the jet radiation significantly…

高能天体物理现象 · 物理学 2020-07-07 Filippo D'Ammando

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

Narrow-line Seyfert 1 galaxies (NLS1s) exhibit extreme soft X-ray excess and large variability. We argue that both features can be basically accounted for by the slim disk model. We assume that a central black-hole mass in NLS1 is…

天体物理学 · 物理学 2015-06-24 Shin Mineshige , Toshihiro Kawaguchi , Mitsuru Takeuchi , Kiyoshi Hayashida

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

It is not yet well known whether narrow line Seyfert 1 (NLS1) galaxies follow the $M_{BH} - \sigma_{\star}$ relation found for normal galaxies. Emission lines, such as [SII] or [OIII]$\lambda$5007, have been used as a surrogate of the…

星系天体物理 · 物理学 2016-12-14 Eduardo O. Schmidt , Diego Ferreiro , Luis Vega , Gabriel A. Oio

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 have used the ROSAT Bright Source Catalogue to extract a complete sample of sources selected in the band from 0.1-0.4 keV. This 1/4 keV-selected sample is comprised of 54 Seyfert galaxies, 25 BL Lacertae objects, 4 clusters and 27…

天体物理学 · 物理学 2008-11-26 S. Vaughan , R. Edelson , R. S. Warwick , M. A. Malkan , M. R. Goad

Radio-loud Narrow-line Seyfert 1 (NLS1) galaxies are unique probes of the formation of powerful radio jets at extreme (near-Eddington) accretion rates and low black hole masses, in a regime very different from classical blazars and,…

星系天体物理 · 物理学 2018-08-07 S. Komossa

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 use publicly available XMM-Newton data to systematically compare the hard X-ray photon indices, $\Gamma_{\rm 2-10\ keV}$ and the iron K$\alpha$ emission lines of narrow-line (NL) and broad-line Seyfert 1 (BLS1) galaxies. We compile a…

星系天体物理 · 物理学 2010-11-29 Xin-Lin Zhou , Shuang-Nan Zhang

There is growing evidence to suggest that the black hole mass has been previously underestimated with the H$\beta$ line width for certain active galactic nuclei (AGN). With the assumption of the flatter rather than isotropic velocity…

星系天体物理 · 物理学 2016-06-21 Xiang Liu , Pingping Yang , Renzhi Su , Zhen Zhang

Based on photoionization calculations we present a study of the NLR emission line ratios of Narrow-line Seyfert 1 (NLS1) galaxies. In particular, we investigate the influence of different EUV - soft-X-ray spectral shapes (a giant soft…

天体物理学 · 物理学 2007-05-23 S. Komossa , D. Grupe , M. Janek

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

The ROSAT Ultradeep HRI survey in the Lockman Hole contains a complete sample of 91 X-ray sources with fluxes in the 0.5-2 keV band larger than 1.2 times 10e-15 erg cm-2 s-1, where over about 75 per cent of the sources are quasars or…

天体物理学 · 物理学 2009-10-31 G. Hasinger , I. Lehmann , M. Schmidt , J. E. Gunn , D. P. Schneider , R. Giacconi , J. Truemper , G. Zamorani

Narrow-line Seyfert 1 galaxies (NLS1s) are active galactic nuclei (AGN) recently identified as a new class of $\gamma$-ray sources. The high energy emission is explained by the presence of a relativistic jet observed at small angles, just…

This is the first paper in a series dedicated to the study of the emission-line and continuum properties of narrow line Seyfert 1 galaxies (NLS1s). We carried out a systematic search for NLS1s from objects assigned as ``QSOs'' or…

天体物理学 · 物理学 2009-07-28 Hongyan Zhou , Tinggui Wang , Weimin Yuan , Honglin Lu , Xiaobo Dong , Junxian Wang , Youjun Lu

We present a sample of 150 narrow-line Seyfert 1s (NLS1s) found within the Sloan Digital Sky Survey Early Data Release (EDR), only two of which were previously identified as such. This substantially increases the known number of NLS1s, and…

天体物理学 · 物理学 2009-11-07 Rik J. Williams , Richard W. Pogge , Smita Mathur

This work studies the optical emission line properties and physical conditions of the narrow line region (NLR) of seven narrow-line Seyfert 1 galaxies (NLS1). Our results show that the flux carried out by the narrow component of H-beta is,…

天体物理学 · 物理学 2009-10-31 A. Rodriguez-Ardila , L. Binette , M. G. Pastoriza , C. J. Donzelli , .

Recently growing evidence has been accumulated that the NLS1s are viewed from nearly pole-on viewing angles. However, there has been no theoretical model which explains the following important correlations; 1) weaker optical Fe II emitters…

天体物理学 · 物理学 2007-05-23 Yoshiaki Taniguchi , Takashi Murayama , Tohru Nagao

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…