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Related papers: Narrow-Line Seyfert 1 Galaxies

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In this paper, we explore the physics of the accretion and jet in narrow-line Seyfert 1 galaxies (NLS1). Specifically, we compile a sample composed of 16 nearby NLS1 with $L_{\rm bol}/L_{\rm Edd} \gtrsim 0.1$. We investigate the mutual…

High Energy Astrophysical Phenomena · Physics 2018-04-11 Su Yao , Erlin Qiao , Xue-Bing Wu , Bei You

We propose two statistical tests to investigate how we see the nuclear region (r < 0.1 pc) of Narrow-Line Seyfert 1 galaxies (NLS1s). 1) The high-ionization nuclear emission-line region (HINER) test: Seyfert 1 galaxies (S1s) have…

Astrophysics · Physics 2009-10-31 T. Murayama , T. Nagao , Y. Taniguchi

Narrow-line Seyfert 1 (NLS1) galaxies are believed to be active galactic nuclei (AGN) in the early stages of their evolution. Some dozens of them have been found to host relativistic jets, whilst the majority has not even been detected in…

Astrophysics of Galaxies · Physics 2022-01-26 Emilia Järvelä , Rohan Dahale , Luca Crepaldi , Marco Berton , Enrico Congiu , Robert Antonucci

We report a detailed analysis of the XMM-Newton spectra of six Narrow-Line Seyfert 1 (NLS1) galaxies at redshift z = 0.35--0.92. Compared with the NLS1s at lower redshift in the previously most-studied sample, these NLS1s have larger black…

High Energy Astrophysical Phenomena · Physics 2023-05-25 Zhibo Yu , Jiachen Jiang , Cosimo Bambi , Luigi C. Gallo , Dirk Grupe , Andrew C. Fabian , Christopher S. Reynolds , William N. Brandt

Narrow-line Seyfert 1 galaxies (NLS1s) are an interesting subclass of active galactic nuclei (AGN), which tipically does not exhibit any strong radio emission. Seven percent of them, though, are radio-loud and often show a flat…

Using the BH masses deduced from the empirical relation of Kaspi et al. (2000) and assuming that the optical luminosity is provided by the accretion disc, we show that Narrow Line Seyfert Galaxies 1 (NLS1s) accrete at super-Eddington rates,…

Astrophysics · Physics 2009-11-10 S. Collin , Toshihiro Kawaguchi

Recent X-ray observations have advanced the study of ultrasoft Narrow-Line Seyfert 1 galaxies and have revealed strikingly clear correlations between optical emission line properties and the shape of the X-ray continuum. In particular, the…

Astrophysics · Physics 2007-05-23 W. N. Brandt , Th. Boller

We obtained 0.8-2.4 micron spectra at a resolution of 320 km/s of four narrow-line Seyfert 1 galaxies in order to study the near-infrared properties of these objects. We focus on the analysis of the FeII emission in that region and the…

Astrophysics · Physics 2009-11-07 A. Rodriguez-Ardila , S. M. Viegas , M. G. Pastoriza , L. Prato

We report finding kiloparsec-scale radio emissions aligned with parsec-scale jet structures in the narrow-line Seyfert 1 (NLS1) galaxy Mrk 1239 using the Very Large Array and the Very Long Baseline Array. Thus, this radio-quiet NLS1 has a…

Astrophysics of Galaxies · Physics 2015-06-23 Akihiro Doi , Kiyoaki Wajima , Yoshiaki Hagiwara , Makoto Inoue

We present HST/ACS observations of ten galaxies that host narrow-line Seyfert 1 (NLS1) nuclei, believed to contain relatively smaller mass black holes accreting at high Eddington ratios. We deconvolve each ACS image into a nuclear point…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Smita Mathur , Dale Fields , Bradley M. Peterson , Dirk Grupe

Based on a new spectroscopic sample observed using the WHT, we examine the kinematic properties of the various emission line regions in narrow line Seyfert 1 galaxies (NLS1s) by modelling their profiles using multiple component fits. We…

Astrophysics · Physics 2009-11-13 James R. Mullaney , Martin J. Ward

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…

We present a new catalog of narrow-line Seyfert 1 (NLSy1) galaxies from the Sloan Digital Sky Survey Data Release 12 (SDSS DR12). This was obtained by a systematic analysis through modeling of the continuum and emission lines of the spectra…

Astrophysics of Galaxies · Physics 2017-04-26 Suvendu Rakshit , C. S. Stalin , Hum Chand , Xue-Guang Zhang

The evolutionary role of the so-called ``changing-look'' (CL) active galactic nucleus (AGN), which is characterized by spectral-type transitions within $\sim10$ yr, has been suggested in the past few years. By focusing on CL-AGNs having…

Astrophysics of Galaxies · Physics 2026-03-24 J. Wang , S. Jin , D. W. Xu , WeiKang Zheng , Thomas G. Brink , S. Komossa , 1 Alexei V. Filippenko , J. Y. Wei

We study the narrow-line region (NLR) of six Seyfert-1 and six Seyfert-2 galaxies by means of spatially resolved optical spectroscopy and photoionization modelling. From spatially resolved spectral diagnostics, we find a transition between…

Astrophysics · Physics 2007-05-23 Nicola Bennert , Bruno Jungwiert , Stefanie Komossa , Martin Haas , Rolf Chini , ;

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…

Astrophysics · Physics 2007-05-23 K. P. Singh , L. R. Jones

We investigate the relation between the X-ray nuclear emission, optical emission line, radio luminosity and black hole mass for a sample of nearby Seyfert galaxies. Strong linear correlations between the 2-10 keV and [OIII], radio…

Astrophysics · Physics 2008-11-26 F. Panessa , L. Bassani , M. Cappi , M. Dadina , X. Barcons , F. J. Carrera , L. C. Ho , K. Iwasawa , S. Pellegrini

We present part of the results from a spectroscopic monitoring programme on a sample of AGNs, relative to Narrow Line Seyfert 1 Galaxies: following the idea that Balmer-line variability can help discriminate among the possible models for…

Astrophysics · Physics 2007-05-23 M. Ester Giannuzzo , Marco Mignoli , Giovanna M. Stirpe , Andrea Comastri

Narrow-line Seyfert 1 galaxies (NLS1s) are a class of active galactic nuclei (AGN) which are known to be one of the few sources of $\gamma$ rays, which originate in a relativistic beamed jet. Becuase of their relatively large distance, a…

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