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Related papers: III Zw 2, the first superluminal jet in a Seyfert …

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So far, all relativistically boosted jets with superluminal motion have only been detected in typical radio galaxies with early type host galaxies. We have now discovered superluminal motion in the Seyfert I galaxy III Zw 2, classified as a…

Astrophysics · Physics 2007-05-23 A. Brunthaler , H. Falcke , G. C. Bower , M. F. Aller , H. D. Aller , H. Teraesranta

A very detailed monitoring of a radio flare in the Seyfert I galaxy III Zw 2 with the VLA and the VLBA is presented. The relative astrometry in the VLBA observations was precise on a level of a few microarcseconds. Spectral and spatial…

Astrophysics · Physics 2007-05-23 A. Brunthaler , H. Falcke , G. C. Bower , M. F. Aller , H. D. Aller , H. Teraesranta

III Zw 2 is a spiral galaxy with an optical spectrum and faint extended radio structure typical of a Seyfert galaxy, but also with an extremely variable, blazar-like radio core. We have now discovered a new radio flare where the source has…

The afterglow of the binary neutron star merger GW170817 gave evidence for a structured relativistic jet and a link between such mergers and short gamma-ray bursts. Superluminal motion, found using radio very long baseline interferometry…

High Energy Astrophysical Phenomena · Physics 2022-10-14 Kunal P. Mooley , Jay Anderson , Wenbin Lu

We report on X-ray observations of the radio-intermediate, X-ray bright Seyfert 1 galaxy, III Zw 2, obtained with XMM-Newton, Suzaku, and Swift over the past 17-years. The source brightness varies significantly over yearly time scales, but…

High Energy Astrophysical Phenomena · Physics 2017-12-05 Adam G. Gonzalez , Sophia G. H. Waddell , Luigi C. Gallo

Faster-than-light or superluminal motion was originally predicted as a relativistic illusion of ballistic moving ejecta, and confirmed in a few tens of sources observationally. However, the recent results of the long-term multi-epoch…

Astrophysics · Physics 2009-11-13 Biping Gong

AGNs with hard $\gamma$-ray emission identified so far are radio-loud. III Zw 2 is a radio intermediate AGN with a relativistic jet. We study its spectral energy distribution (SED) and find that the broad band emissions are dominated by the…

High Energy Astrophysical Phenomena · Physics 2010-09-09 Liang Chen , J. M. Bai , Jin Zhang , H. T. Liu

Narrow-line Seyfert 1 (NLS1) galaxies are a peculiar subclass of active galactic nuclei (AGN). Among them, TXS 1206+549 belongs to a small group of radio-loud and gamma-ray-emitting NLS1 galaxies. We focus on the radio properties of this…

High Energy Astrophysical Phenomena · Physics 2024-02-20 Bettina Kozák , Sándor Frey , Krisztina Éva Gabányi

We report the detection of an optical jet in the nearby Seyfert 1 radio galaxy 3C 120. The optical jet coincides with the well-known radio jet and emits continuum radiation (B,V',I) with a radio-to-optical spectral index of 0.65. There are…

Astrophysics · Physics 2008-02-03 J. Hjorth , M. Vestergaard , A. N. Sorensen , F. Grundahl

Disk winds and jets are ubiquitous in active galactic nuclei (AGN), and how these two components interact remains an open question. We study the radio properties of a radio-intermediate quasar III Zw 2. We detect two jet knots J1 and J2 on…

III Zw 2 is the prototype of radio-intermediate quasars. Although there is the evidence of possessing strong jet, significant $\gamma$-ray emission has not been reported before. In this work, we carry out a detailed analysis of the latest…

High Energy Astrophysical Phenomena · Physics 2016-10-19 Neng-Hui Liao , Yu-Liang Xin , Xu-Liang Fan , Shan-Shan Weng , Shao-Kun Li , Liang Chen , Yi-Zhong Fan

We report superluminal jet motion with an apparent speed of $\beta_\mathrm{app}=1.65\pm0.57$ in the radio-quiet (RQ) low ionisation nuclear emission line region (LINER) galaxy, KISSR872. This result comes from two epoch phase-referenced…

X-ray spectral timing analysis is presented of XMM-Newton observations of the narrow line Seyfert 1 galaxy I Zwicky 1 (I Zw 1) taken in 2015 January. After exploring the effect of background flaring on timing analyses, X-ray time lags…

High Energy Astrophysical Phenomena · Physics 2017-09-06 D. R. Wilkins , L. C. Gallo , C. V. Silva , E. Costantini , W. N. Brandt , G. A. Kriss

II Zw 40 is a starburst dwarf and merger product, and holds a radio-infrared supernebula excited by thousands of embedded OB stars. We present here observations of three aspects of the supernebula: maps of the K and KU radio continuum that…

Astrophysics of Galaxies · Physics 2024-10-24 Dan Beilis , Sara Beck , John Lacy , Jean L. Turner , Hauyu Baobab Liu , Paul T. P. Ho , S. Michelle Consiglio

We have obtained HST FOC long-slit optical spectroscopy of the Narrow Line Region of the Seyfert 2 galaxy Mrk 3. In the region cospatial with the radio-jet the velocity field is highly perturbed and shows two velocity systems separated by…

Astrophysics · Physics 2009-10-31 A. Capetti , D. J. Axon , F. D. Macchetto , A. Marconi , C. Winge

We present results based on an XMM-Newton observation of the prototype narrow-line Seyfert 1 galaxy I Zw 1 performed in June 2002. The 0.6-12 keV spectrum is well described by a steep power-law (Gamma\sim 2.3) and a weak soft blackbody…

Astrophysics · Physics 2007-05-23 G. C. Dewangan , R. E. Griffiths

Using newly released data from the Wide-field Infrared Survey Explorer, we report the discovery of rapid infrared variability in three radio-loud narrow-line Seyfert 1 galaxies (NLS1s) selected from the 23 sources in the sample of Yuan et…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Ning Jiang , Hong-Yan Zhou , Luis C. Ho , Weimin Yuan , Ting-Gui Wang , Xiao-Bo Dong , Peng Jiang , Tuo Ji , Qiguo Tian

The nearby dwarf galaxy II Zw 40 hosts an intense starburst. At the center of the starburst is a bright compact radio and infrared source, thought to be a giant dense HII region containing ~14,000 O stars. Radio continuum images suggest…

Astrophysics of Galaxies · Physics 2015-06-15 Sara Beck , Jean Turner , John Lacy , Thomas Greathouse , Ohr Lahad

We investigate the relativistic jet of the powerful radio-emitting blazar J1429+5406 at redshift z=3.015. Our understanding of jet kinematics in z>3 quasars is still rather limited, based on a sample of less than about 50 objects. The…

Astrophysics of Galaxies · Physics 2025-05-14 Dávid Koller , Sándor Frey

We present the results of 5 GHz VLBI observations of a compact steep spectrum source 3C 138. The data are consistent with the western end being the location of the central activity. The observed offset between different frequencies in the…

Astrophysics · Physics 2009-11-06 Z. -Q. Shen , D. R. Jiang , S. Kameno , Y. J. Chen
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