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The idea that some of the unusual features in the X-ray spectra of Narrow-Line Seyfert 1 galaxies (NLS1s) are due to the steep X-ray continuum is tested by comparing photoionization model calculations with various observed properties of…

天体物理学 · 物理学 2009-10-31 Hagai Netzer

The excellent soft X-ray sensitivity of the PSPC detector onboard the ROSAT satellite provided the first chance to study precisely the spectral and timing properties of Narrow-Line Seyfert 1 galaxies. ROSAT observations of Narrow-Line…

天体物理学 · 物理学 2009-10-31 Th. Boller

Narrow-line Seyfert 1 galaxies (NLSy1s) are a subclass of active galactic nuclei (AGNs), commonly associated with rapidly accreting, relatively low-mass black holes ($10^6$ - $10^8 M_\odot$) hosted in spiral galaxies. Although typically…

星系天体物理 · 物理学 2025-11-26 Rachana , M. Vivek , Yue Shen

Narrow-line Seyfert 1 galaxies (NLS1) are an intriguing subclass of active galactic nuclei. Their observed properties indicate low central black hole mass and high accretion rate. The extremely radio-loud NLS1 sources often show…

星系天体物理 · 物理学 2017-11-07 K. É. Gabányi , S. Frey , Z. Paragi , E. Järvelä , T. Morokuma , T. An , M. Tanaka , I. Tar

AGNs with narrow Balmer lines show various extreme properties. In particular, rapid X-ray variability, steep X-ray spectra, peculiar optical and UV line ratios, and possibly peculiar line profiles. Since all these phenomena occur together…

天体物理学 · 物理学 2009-10-31 Ari Laor

We extend the analysis presented in Tran (2001) of a spectropolarimetric survey of the CfA and 12micron samples of Seyfert 2 galaxies (S2s). We confirm that S2s with hidden broad line regions (HBLRs) tend to have hotter circumnuclear dust…

天体物理学 · 物理学 2009-11-07 Hien D. Tran

As one of the drivers of feedback in active galactic nuclei (AGNs), the jets launched from supermassive black holes (SMBHs) are important for understanding the co-evolution of SMBHs and their host galaxies. However, the formation of AGN…

高能天体物理现象 · 物理学 2023-06-06 Su Yao , S. Komossa

We study the properties of infrared-selected QSOs (IR QSOs), optically-selected QSOs (PG QSOs) and Narrow Line Seyfert 1 galaxies (NLS1s). We compare their properties from the infrared to the optical and examine various correlations among…

天体物理学 · 物理学 2008-11-26 C. N. Hao , X. Y. Xia , Shude Mao , Hong Wu , Z. G. Deng

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…

天体物理学 · 物理学 2007-05-23 Nicola Bennert , Bruno Jungwiert , Stefanie Komossa , Martin Haas , Rolf Chini , ;

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,…

天体物理学 · 物理学 2009-11-10 S. Collin , Toshihiro Kawaguchi

We present the first multi-parameter analysis of the narrow line AGN clustering properties. Estimates of the two-point correlation function (CF) based on SDSS DR2 data reveal that Seyferts are clearly less clustered than normal galaxies,…

天体物理学 · 物理学 2011-02-11 Anca Constantin , Michael S. Vogeley

We present spectroscopic observations of 27 active galactic nuclei (AGN) with some of the lowest black hole (BH) masses known. We use the high spectral resolution and small aperture of our Keck data, taken with the Echellette Spectrograph…

宇宙学与河外天体物理 · 物理学 2015-06-11 Randi R. Ludwig , Jenny E. Greene , Aaron J. Barth , Luis C. Ho

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

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

Why are the nuclei of some galaxies more active than others? If most galaxies harbor a central massive black hole, the main difference is probably in how well it is fueled by its surroundings. We investigate the hypothesis that such a…

天体物理学 · 物理学 2009-11-10 L. K. Hunt , M. A. Malkan

We present black hole mass--bulge velocity dispersion relation for a complete sample of 75 soft X-ray selected AGNs: 43 broad line Seyfert 1s and 32 narrow line Seyfert 1s. We use luminosity and FWHM(H-beta) as surrogates for black hole…

天体物理学 · 物理学 2009-11-10 Dirk Grupe , Smita Mathur

1H0323+342 is one of narrow-line radio-loud Seyfert 1 galaxies (RL-NLS1), which is a new class of gamma-ray emitting AGNs. Narrow-line Seyfert 1 galaxies (NLS1) have a small-mass black hole, but its mass accretion rate is almost as high as…

高能天体物理现象 · 物理学 2015-03-12 H. Shirakawa , Y. Fukazawa , Y. Tanaka , R. Itoh , K. Kawaguchi

A sample of narrow-line (NLS1) and broad-line Seyfert 1 (BLS1) galaxies observed with Suzaku is presented. The final sample consists of 22 NLS1s and 47 BLS1s, for a total of 69 AGN that are all at low redshift (z<0.5) and exhibit low host…

高能天体物理现象 · 物理学 2020-10-07 Sophia G. H. Waddell , Luigi C. Gallo

In recent years, several Radio-Loud Narrow-Line Seyfert 1 galaxies (RL-NLS1) possessing relativistic jets have come into attention with their detections in Very Large Baseline Array (VLBA) and in $\gamma$-ray observations. In this paper we…

星系天体物理 · 物理学 2018-07-09 Veeresh Singh , Hum Chand

We present the first systematic study of (non-radio-selected) radio-loud narrow-line Seyfert 1 (NLS1) galaxies. Cross-correlation of the `Catalogue of Quasars and Active Nuclei' with several radio and optical catalogues led to the…

天体物理学 · 物理学 2008-11-26 S. Komossa , W. Voges , D. Xu , S. Mathur , H. -M. Adorf , G. Lemson , W. Duschl , D. Grupe