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相关论文: Large-scale environments of narrow-line Seyfert 1 …

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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

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…

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

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…

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…

星系天体物理 · 物理学 2022-01-26 Emilia Järvelä , Rohan Dahale , Luca Crepaldi , Marco Berton , Enrico Congiu , Robert Antonucci

Narrow-line Seyfert 1 (NLS1) galaxies provide us with unique insights into the drivers of AGN activity under extreme conditions. Given their low black hole (BH) masses and near-Eddington accretion rates, they represent a class of galaxies…

高能天体物理现象 · 物理学 2017-06-28 V. Karamanavis , E. Angelakis , S. Komossa , I. Myserlis , D. Blinov , J. A. Zensus

We study a sample of Narrow-line Seyfert 1 galaxies (NLS1) in their optical and radio features, in order to understand the differences between their radio silent, radio-loud and radio-quiet subclasses. We first show that the different…

星系天体物理 · 物理学 2018-08-15 Tullia Sbarrato , Massimo Dotti , Giancarlo Ghirlanda , Fabrizio Tavecchio

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

Narrow-line Seyfert 1 (NLS1) galaxies are active galactic nuclei (AGN) believed to be in the early stages of their evolution. A fraction of them have been found to host relativistic jets. Due to the lack of large-scale diffuse radio…

星系天体物理 · 物理学 2021-08-20 Emilia Järvelä , Marco Berton , Luca Crepaldi

The last decade has witnessed a steadily increasing number of observational studies concerning the rare class of radio loud narrow-line Seyfert 1 galaxies, of which several hundred are currently known. According to the current AGN paradigm,…

星系天体物理 · 物理学 2018-05-15 Matthew L. Lister

Narrow-line Seyfert 1 galaxies, with their extreme properties, defy our current knowledge of active galactic nuclei and relativistic jet systems. They excite, and might help us answer, many questions concerning the evolution and unification…

星系天体物理 · 物理学 2016-03-15 Emilia Järvelä , Anne Lähteenmäki

We report the first results of a survey on 74 narrow-line Seyfert 1 galaxies (NLS1s) carried out in 2015 with the Karl G. Jansky Very Large Array (JVLA) at 5 GHz in A-configuration. So far, this is the largest survey aimed to image the…

A fraction of Narrow Line Seyfert 1 galaxies (NLS1) are hosted by galaxies that present a disturbed morphology, in some cases hinting for merger processes, that are putative sources of gas replenishment. We have been investigating the…

星系天体物理 · 物理学 2018-09-06 Sonia Anton , Alessandro Caccianiga , Luca Bizzocchi , Jose Afonso

Narrow-Line Seyfert 1 galaxies (NLS1s) are generally believed to be radio-quiet Active Galactic Nuclei (AGN) with relatively less-massive (10$^{5}$$-$10$^{8}$~M$_{\odot}$) Super-Massive Black Holes (SMBH). Using the FIRST radio detections…

星系天体物理 · 物理学 2018-07-16 Veeresh Singh , Hum Chand , C. H. Ishwara-Chandra , Preeti Kharb

We present results from the analysis of the optical spectra of 47 radio-selected narrow-line Seyfert 1 galaxies (NLS1s). These objects are a subset of the First Bright Quasar Survey (FBQS) and were initially detected at 20 cm (flux density…

天体物理学 · 物理学 2008-11-26 D. J. Whalen , S. A. Laurent-Muehleisen , E. C. Moran , R. H. Becker

Thanks to the execution of extensive spectroscopic surveys that have covered large fractions of the sky down to magnitudes as faint as $i \approx 19$, it has been possible to identify several narrow-line Seyfert 1 galaxies (NLS1s) and to…

星系天体物理 · 物理学 2018-09-10 G. La Mura , D. Bastieri , M. Berton , S. Chen , S. Ciroi , E. Congiu , V. Cracco , J. -H. Fan , P. Rafanelli

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…

We present a statistical study of a large, homogeneously analyzed sample of narrow-line Seyfert 1 (NLS1) galaxies, accompanied by a comparison sample of broad-line Seyfert 1 (BLS1) galaxies. Optical emission-line and continuum properties…

宇宙学与河外天体物理 · 物理学 2015-06-03 Dawei Xu , S. Komossa , Hongyan Zhou , Honglin Lu , Cheng Li , Dirk Grupe , Jing Wang , Weimin Yuan

Narrow-line Seyfert 1 galaxies (NLS1s), a subclass of active galactic nuclei (AGNs) at early stage of accretion process, are also found to host relativistic jets. However, currently known jetted NLS1s are rare. The majority of NLS1s are…

星系天体物理 · 物理学 2024-02-23 Xu-Liang Fan

(abridged) We present a comprehensive study of a sample of 23 genuine radio-loud NLS1 galaxies which have the radio-loudness parameters greater than 100. The radio sources of the sample are ubiquitously compact. A significant fraction of…

天体物理学 · 物理学 2009-11-13 W. Yuan , H. Y. Zhou , S. Komossa , X. B. Dong , T. G. Wang , H. L. Lu , J. M. Bai
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