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Related papers: Coronal Line Emission from NLS1s

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We combine emission line and X-ray luminosities for 45 sources from the Chandra Deep Field South (CDF-S), and seven HELLAS sources, to obtain a new sample of 52 X-ray selected type-II active galactic nuclei (AGNs). Eighteen of our sources…

Astrophysics · Physics 2009-11-11 Hagai Netzer , V. Mainieri , P. Rosati , Benny Trakhtenbrot

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

We present a detailed comparative systematic study using a sample of 221 Narrow-line Seyfert 1 (NLSy1) galaxies in comparison to a redshift matched sample of 154 Broad-line Seyfert 1 (BLSy1) galaxies based on their observations using ROSAT…

High Energy Astrophysical Phenomena · Physics 2020-06-24 Vineet Ojha , Hum Chand , Gulab Chand Dewangan , Suvendu Rakshit

We report the discovery and analysis of the follow-up ROSAT pointed observation, an ASCA observation and optical and radio observations of the enigmatic Narrow-Line Seyfert 1 galaxy RX J0134.2-4258. While its spectrum was one of the softest…

Astrophysics · Physics 2007-05-23 D. Grupe , K. M. Leighly , H. -C. Thomas , S. A. Laurent-Muehleisen

In this work we present a multiwavelength study of narrow-line Seyfert 1 galaxies (NLS1s) discovered in the Second Byurakan Survey (SBS). The sample consists of 26 objects, which have $M_{B}\ge -23.0$, or $-19.9 > M_{B} > -23.0$, $0.0243 <…

We present a detailed analysis of the XMM-Newton observations of five narrow-line Seyfert 1 galaxies (NLS1s). They all show very soft continuum emission in the X-ray band with a photon index of $\Gamma\gtrsim 2.5$. Therefore, they are…

High Energy Astrophysical Phenomena · Physics 2022-05-18 Jiachen Jiang , Luigi C. Gallo , Andrew C. Fabian , Michael L. Parker , Christopher S. Reynolds

We present an analysis of the X-ray variability properties of the NLS1 galaxy Ton S180, based upon a 12-day continuous ASCA observation. We observe flux variations of a factor of 3.5 in the 0.7-1.3 keV band and 3.9 in the 2-10 keV…

Astrophysics · Physics 2008-11-26 P. Romano , T. J. Turner , S. Mathur , I. M. George

We present joint \textit{XMM-Newton} and \textit{NuSTAR} observations of the `bare' narrow line Seyfert 1 Ton S180 ($z=0.062$), carried out in 2016 and providing the first hard X-ray view of this luminous galaxy. We find that the 0.4--30…

We present an accurate characterisation of the high-resolution X-ray spectrum of the Narrow Line Seyfert 1 galaxy Arakelian 564 and put it in to context with other objects of its type by making a detailed comparison of their spectra. The…

Astrophysics · Physics 2009-11-13 R. A. N. Smith , M. J. Page , G. Branduardi-Raymont

Forbidden coronal lines has traditionally called the attention due to the high-energy photons required for their production (IP $>$100~eV, where IP is the ionisation potential of the transitions that originate the line). As such, they are…

Astrophysics of Galaxies · Physics 2025-02-11 Alberto Rodriguez-Ardila , Fernando Cerqueira-Campos

Seyfert galaxies have been shown to exhibit a large variety of features in their X-ray spectra from which the environment of the central engine can be deduced. We focus on the two following aspects: the Warm Absorber, mainly responsible of…

Astrophysics · Physics 2007-05-23 M. Mouchet , A. Abrassart , D. Porquet , A. -M. Dumont , S. Collin

Coronal lines are a powerful, yet poorly understood, tool to identify and characterize Active Galactic Nuclei (AGNs). There have been few large scale surveys of coronal lines in the general galaxy population in the literature so far. Using…

Astrophysics of Galaxies · Physics 2023-03-08 Michael Reefe , Remington O. Sexton , Sara M. Doan , Shobita Satyapal , Nathan J. Secrest , Jenna M. Cann

[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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 A. Tarchi , P. Castangia , A. Columbano , F. Panessa , J. A. Braatz

A long 280 ks observation of the Seyfert 1 galaxy NGC 3783 with XMM-Newton is reported. We focus on the oxygen line complex between 17 and 24 A as measured with the RGS spectrometers. Accurate absorption column densities and emission line…

Ultra-soft narrow line Seyfert 1 (US-NLSy) are a poorly observed class of active galactic nuclei characterized by significant flux changes and an extreme soft X-ray excess. This peculiar spectral shape represents a golden opportunity to…

In recent years there have been many reported detections of highly redshifted or blueshifted narrow spectral lines (both emission or absorption) in the X-ray spectra of active galaxies, but these are all modest detections in terms of their…

Astrophysics · Physics 2009-11-13 S. Vaughan , P. Uttley

We present {\it ASCA} observations of the Seyfert 1 galaxies Mrk~1040 and MS~0225.5+3121. Mrk~1040 was found to have decreased in flux by almost a factor of 4 since an {\it EXOSAT} observation 10\,years ago. The energy spectrum of Mrk~1040…

Astrophysics · Physics 2015-06-24 C. S. Reynolds , A. C. Fabian , H. Inoue

We present the broad-band soft and hard X-ray spectral analysis of 8 Narrow Line Seyfert 1 galaxies extracted from the IBISCO Sample. The study also focuses on the properties of the NLS1 in our sample in relation to those of the IBISCO…

High Energy Astrophysical Phenomena · Physics 2018-07-17 Manuela Molina , Angela Malizia , Fabrizio Fiore , Chiara Feruglio

The properties of narrow-line Seyfert 1 (NLS1) galaxies, the links and correlations between them, and the physics behind them, are still not well understood. Apart from accretion rates and black hole masses, density and outflows were…

Astrophysics · Physics 2009-11-13 Dawei Xu , Stefanie Komossa , Hongyan Zhou , Tinggui Wang , Jianyan Wei

High-energy {\gamma}-rays, which are produced by powerful relativistic jets, are usually associated with blazars and radio galaxies. In the current active galactic nuclei (AGN) paradigm, such jets are almost exclusively launched from…

Astrophysics of Galaxies · Physics 2014-12-24 Emilia Järvelä , Anne Lähteenmäki , Jonathan León-Tavares