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相关论文: Jet directions in Seyfert galaxies

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The orientation of radio jets relative to their host galaxies offers an interesting avenue for probing the connection between active galactic nuclei (AGN) and their surroundings. Several studies have also investigated the orientation of…

星系天体物理 · 物理学 2026-02-02 Emma Jane Weller , Pieter van Dokkum

Narrow-line Seyfert 1 (NLS1) galaxies are unevolved active galactic nuclei (AGN) that exist predominantly in spiral galaxies. However, mostly due to the small number of sources studied, it has been under debate whether also the hosts of…

星系天体物理 · 物理学 2022-12-14 Irene Varglund , Emilia Järvelä , Anne Lähteenmäki , Marco Berton , Stefano Ciroi , Enrico Congiu

What triggers collimated relativistic outflows or jets, from the centers of galaxies remains a fundamental question in astrophysics. The merging of two galaxies has been proposed to realize the conditions to successfully launch and drive…

The spectra of active galactic nuclei usually exhibit wings in some emission lines, such as [OIII]$\lambda\lambda$5007,4959, with these wings generally being blueshifted and related to strong winds and outflows. The aim of this work was to…

星系天体物理 · 物理学 2021-02-03 Eduardo O. Schmidt , Laura D. Baravalle , Adriana R. Rodríguez-Kamenetzky

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…

This article combines new CCD polarimetric data with previous information about protostellar objects in a search for correlations involving the interstellar magnetic field. Specifically, we carried out an optical polarimetric study of a…

太阳与恒星天体物理 · 物理学 2011-11-24 Cristiane G. Targon , Claudia V. Rodrigues , Adriano H. Cerqueira , Gabriel R. Hickel

We studied seven nearby narrow-line Seyfert 1 (NLS1) galaxies in $J$- and $Ks$-bands with redshifts varying from 0.019 to 0.092. This is the first multi-source study targeting the hosts of southern NLS1 galaxies. Our data was obtained with…

星系天体物理 · 物理学 2023-11-01 I. Varglund , E. Järvelä , S. Ciroi , M. Berton , E. Congiu , A. Lähteenmäki , F. Di Mille

This paper presents a statistical analysis of the circumgalactic environment of nearby Seyfert galaxies based on a computer-aided search of companion galaxies on the Digitized Sky Survey (DSS). An intrinsic difference between the…

天体物理学 · 物理学 2009-10-31 D. Dultzin-Hacyan , Y. Krongold , I. Fuentes-Guridi , P. Marziani

We present a sample of 30 wide angle tailed radio galaxies (WATs) that we use to constrain the jet speeds in these sources. We measure the distribution of jet-sidedness ratios for the sample, and assuming that the jets are beamed, jet…

天体物理学 · 物理学 2009-11-11 Nazirah N. Jetha , Martin J. Hardcastle , Irini Sakelliou , .

The $BeppoSAX$ archive is currently the largest reservoir of high sensitivity simultaneous soft and hard-X ray data of Seyfert galaxies. From this database all the Seyfert galaxies (105 objects of which 43 are type I and 62 are type II)…

天体物理学 · 物理学 2009-11-13 Mauro Dadina

Recent observations using several different telescopes and sky surveys showed patterns of asymmetry in the distribution of galaxies by their spin directions as observed from Earth. These studies were done with data imaged from the Northern…

宇宙学与河外天体物理 · 物理学 2021-08-18 Lior Shamir

We present evidence for widespread relativistic effects in the central regions of active galactic nuclei. In a sample of 18 Seyfert 1 galaxies observed by \asca, 14 show an iron K$\alpha$ line which is is resolved, with mean width…

天体物理学 · 物理学 2009-10-28 K. Nandra , I. M. George , R. F. Mushotzky , T. J. Turner , T. Yaqoob

New far-infrared photometry with ISOPHOT, onboard the Infrared Space Observatory, is presented for 58 galaxies with homogeneous published data for another 32 galaxies all belonging to the 12 micron galaxy sample. In total 29 Seyfert 1's, 35…

天体物理学 · 物理学 2009-11-07 Luigi Spinoglio , Paola Andreani , Matthew A. Malkan

We probed the relation between line activities of Seyfert 2 galaxies and their host galaxies. We selected Seyfert 2 galaxies from the Sloan Digital Sky Survey Data Release 10 with redshifts less 0.2. We used the luminosity of the emission…

星系天体物理 · 物理学 2019-03-12 Yen-Chen Chen , Chorng-Yuan Hwang

Because the disc--jet coupling likely depends on various properties of sources probed, the sample control is always an important but challenging task. In this work, we re-analyzed the INTEGRAL hard X-ray-selected sample of Seyfert galaxies.…

高能天体物理现象 · 物理学 2021-03-03 N. Chang , F. G. Xie , X. Liu , L. C. Ho , A. -J. Dong , Z. H. Han , X. Wang

There is theoretical and observational evidence that the jet core position changes with frequency. However, the core position for a given frequency may vary with time in the case of flares or for a precessing jet. In this work, we want to…

高能天体物理现象 · 物理学 2022-04-20 R. Sharma , M. Massi , G. Torricelli-Ciamponi

The problem of Astrophysical Jet formation from relativistic accretion disks through the establishment of relativistic disk-powerful jet equilibrium structure is studied applying the Beltrami-Bernoulli equilibrium approach of Shatashvili &…

高能天体物理现象 · 物理学 2024-06-05 E. Katsadze , N. Revazashvili , N. L. Shatashvili

We argue that the narrow line regions of Seyfert galaxies are powered by the transport of energy and momentum by the radio-emitting jets and consequently that the ratio of the radio power to jet energy flux is much smaller than is usually…

天体物理学 · 物理学 2016-08-30 G. V. Bicknell , M. A. Dopita , Z. Tsvetanov , R. S. Sutherland

We present a study of the cold molecular versus the ionized gas distribution in three nearby Seyfert galaxies: NGC 6860, Mrk 915 and MCG -01-24-012. To constrain the cold molecular flux distribution at $\sim$ 0.5 - 0.8$^{\prime\prime}$…

We analyze differences in positions of active galactic nuclei between Gaia data release 2 and VLBI and compare the significant VLBI-to-Gaia offsets in more than 1000 objects with their jet directions. Remarkably at least 3/4 of the…

星系天体物理 · 物理学 2019-01-30 A. V. Plavin , Y. Y. Kovalev , L. Petrov