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Related papers: AGN-host interaction in IC 5063. I. Large-scale X-…

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We present 21-cm HI line and 13-cm continuum observations, obtained with the Australian Long Baseline Array, of the Seyfert 2 galaxy IC 5063. This object appears to be one of the best examples of Seyfert galaxies where shocks produced by…

Astrophysics · Physics 2009-10-31 T. A. Oosterloo , R. Morganti , A. Tzioumis , J. Reynolds , E. King , P. McCulloch , Z. Tsvetanov

The interstellar medium of the radio galaxy IC 5063 is highly perturbed by an AGN jet expanding in the gaseous disc of the galaxy. We model this interaction with relativistic hydrodynamic simulations and multiphase initial conditions for…

High Energy Astrophysical Phenomena · Physics 2018-07-04 Dipanjan Mukherjee , Alex Y. Wagner , Geoffrey V. Bicknell , Raffaella Morganti , Tom Oosterloo , Nicole Nesvadba , Ralph S. Sutherland

Imaging X-ray spectroscopy of nearby AGNs, mostly with Chandra, has shown that extended soft (<2.5 keV) emission-line dominated X-ray biconical structures, of kiloparsec scale, are widespread in highly absorbed Compton Thick (CT) AGNs. The…

Astrophysics of Galaxies · Physics 2023-04-05 G. Fabbiano , M. Elvis

The biconical radiation pattern extending from an active galactic nucleus (AGN) may strongly photoionize the circumnuclear interstellar medium (ISM) and stimulate emission from the narrow line region (NLR). Observations of the NLR may…

New radio continuum (8 GHz and 1.4 GHz) and HI 21 cm line observations of the Seyfert 2 galaxy IC 5063 (PKS 2048-572) were obtained with the Australia Telescope Compact Array (ATCA). The 8 GHz image reveals a linear triple structure (~4'',…

Astrophysics · Physics 2009-10-30 R. Morganti , T. Oosterloo , Z. Tsvetanov

We report the results of joint Chandra/ACIS - NuSTAR deep observations of NGC 1167, the host galaxy of the young radio jet B2 0258+35. In the ACIS data we detect X-ray emission, extended both along and orthogonal to the jet. At the end of…

High-resolution (0.5 arcsec) CO(2-1) observations performed with the Atacama Large Millimetre/submillimetre Array have been used to trace the kinematics of the molecular gas in the Seyfert 2 galaxy{IC~5063}. Although one of the most…

Astrophysics of Galaxies · Physics 2015-04-21 R. Morganti , T. A. Oosterloo , J. B. R. Oonk , W. Frieswijk , C. N. Tadhunter

Outflows accelerated by AGN are commonly observed in the form of coherent, mildly collimated high-velocity gas directed along the AGN ionisation cones and kinetically powerful (>$10^{44-45}$ erg/s) jets. Recent works found that outflows can…

All the observations available in the Chandra and XMM-Newton archives have been used to investigate the X-ray spectral properties of 3C 33. In this paper is presented a complete X-ray analysis of the nuclear emission of this narrow line…

High Energy Astrophysical Phenomena · Physics 2009-11-13 E. Torresi , P. Grandi , M. Guainazzi , G. G. C. Palumbo , G. Ponti , S. Bianchi

Black hole driven outflows in galaxies hosting active galactic nuclei (AGN) may interact with their interstellar medium (ISM) affecting star formation. Such feedback processes, reminiscent of those seen in massive galaxies, have been…

We present new ATCA 17- and 24-GHz radio images and ESO-NTT optical spectra of the radio-loud Seyfert galaxy IC5063, the first galaxy in which a fast (~ 600 km/s) outflow of neutral hydrogen was discovered. The new radio data confirm the…

Astrophysics · Physics 2009-11-13 R. Morganti , J. Holt , L. Saripalli , T. A. Oosterloo , C. N. Tadhunter

We present a detailed analysis of the XMM-Newton RGS high resolution X-ray spectra of the Seyfert 2 galaxy, Mrk573. This analysis is complemented by the study of the Chandra image, and its comparison to optical (HST) and radio (VLA) data.…

We present a detailed study of the molecular gas in the fast AGN-driven outflow in the nearby radio-loud Seyfert galaxy IC 5063. Using ALMA observations of a number of tracers (12CO(1-0), 12CO(2-1), 12CO(3-2), 13CO(2-1) and HCO+(4-3)), we…

We present our recent results about the extended narrow-line region (ENLR) of two nearby Seyfert 2 galaxies (IC 5063 and NGC 7212) obtained by modelling the observed line profiles and spectra with composite models (photoionization+shocks)…

We present results on Mrk 573 obtained as part of the CHandra survey of Extended Emission-line Regions in nearby Seyfert galaxies (CHEERS). Previous studies showed that this source features a biconical emission in the soft X-ray band…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Alessandro Paggi , Junfeng Wang , Giuseppina Fabbiano , Martin Elvis , Margarita Karovska

We report the discovery with the Atacama Pathfinder EXperiment (APEX) of an outflow of molecular gas in the radio-loud Seyfert galaxy IC5063 (z = 0.0110). In addition to the emission of the large-scale CO disk, a prominent blueshifted wing…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Raffaella Morganti , Wilfred Frieswijk , Raymond J. B. Oonk , Tom Oosterloo , Clive Tadhunter

We present a detailed analysis of the X-ray emission of the Compton-thick (CT) AGN ESO\,137-G034 based on deep ($\sim230$\,ks) Chandra observations. As in other CT AGNs, the morphology of the emission is elongated, approximately following…

High Energy Astrophysical Phenomena · Physics 2026-02-09 D. Ł. Król , G. Fabbiano , M. Elvis , A. Trindade Falcão , R. Middei , D. Rosario , R. Davies , T. Shimizu , D. Hill

To investigate the role of active galactic nucleus (AGN) X-ray irradiation on the interstellar medium (ISM), we systematically analyzed Chandra and ALMA CO($J$=2-1) data for 26 ultra-hard X-ray ($>$ 10 keV) selected AGNs at redshifts below…

Astrophysics of Galaxies · Physics 2021-12-22 Taiki Kawamuro , Claudio Ricci , Takuma Izumi , Masatoshi Imanishi , Shunsuke Baba , Dieu D. Nguyen , Kyoko Onishi

We report four years of radio and X-ray monitoring of the Type IIn supernova SN 2006jd at radio wavelengths with the Very Large Array, Giant Metrewave Radio Telescope and Expanded Very Large Array; at X-ray wavelengths with {\em Chandra},…

We investigate the evolution of active galactic nucleus jets on kiloparsec-scales due to their interaction with the clumpy interstellar medium (ISM) of the host galaxy and, subsequently, the surrounding circumgalactic environment.…

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