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The origin of the low luminosity radio emission in radio-quiet AGN, is unknown. The detection of a positive correlation between the radio and X-ray emission would imply a jet-like origin, similar to that seen in `hard state' X-ray binary…

High Energy Astrophysical Phenomena · Physics 2016-12-21 Sadie Jones , Ian McHardy , Thomas J. Maccarone

We report the results from a six-year, multi-epoch very long baseline interferomertry monitoring of the Seyfert galaxy NGC3079. We have observed NGC3079 during eight epochs between 1999 and 2005 predominantly at 5GHz, but covering the…

Astrophysics · Physics 2008-11-26 Enno Middelberg , Ivan Agudo , Alan L. Roy , Thomas P. Krichbaum

We explore the nature of the radio emission of X-ray selected AGN by combining deep radio (1.4GHz; 60micro-Jy) and X-ray data with multiwavelength (optical, mid-infrared) observations in the Extended Chandra Deep Field South (E-CDFS). The…

We present the first results from a JWST program studying the role played by powerful radio jets in the evolution of the most massive galaxies at the onset of Cosmic Noon. Using NIRSpec integral field spectroscopy, we detect 24 rest-frame…

We present Chandra X-ray results for the jet, nucleus, and gaseous atmosphere of NGC 315, a nearby radio galaxy whose jet kinematics are known through deep radio mapping. Diffuse X-ray synchrotron emission is detected from the jet out to 30…

Astrophysics · Physics 2009-11-13 D. M. Worrall , M. Birkinshaw , R. A. Laing , W. D. Cotton , A. H. Bridle

We report on the nuclear X-ray properties of the radio galaxy NGC 6251 observed with XMM-Newton. NGC 6251 is a well-known radio galaxy with intermediate FRI/II radio properties. It is optically classified as a Seyfert 2 and hosts a…

Astrophysics · Physics 2009-11-10 M. Gliozzi , R. M. Sambruna , W. N. Brandt , R. Mushotzky , M. Eracleous

We report X-ray imaging of the powerful FR-II radio galaxy 3C353 using the Chandra X-ray Observatory. 3C353's two 4"-wide and 2'-long jets allow us to study in detail the internal structure of the large-scale relativistic outflows at both…

We present mid-infrared data of a sample of 57 AGNs obtained with the instrument ISOCAM on board the satellite ISO. The images were obtained through the LW2 (6.75 microns) and LW7 (9.62 microns) filters. This is a new analysis of Clavel et…

We present a detailed, photoionization modeling analysis of XMM-Newton/Reflection Grating Spectrometer observations of the Seyfert 2 galaxy NGC 1068. The spectrum, previously analyzed by Kinkhabwala et al. (2002), reveals a myriad of…

Astrophysics of Galaxies · Physics 2015-06-23 S. B. Kraemer , N. Sharma , T. J. Turner , Ian M. George , D. Michael Crenshaw

We performed a detailed analysis of the Chandra and HST images of the Seyfert 2 galaxy, NGC7582. The dust lane, as mapped by the HST NIR and optical images, strongly influences the morphology of the soft X-ray emission, being spatially…

Astrophysics · Physics 2008-11-26 Stefano Bianchi , Marco Chiaberge , Enrico Piconcelli , Matteo Guainazzi

An increasing number of observations and simulations suggests that low-power (<10$^{44}$ erg s$^{-1}$) jets may be a significant channel of feedback produced by active galactic nuclei (AGN), but little is known about their actual effect on…

We present soft X-ray results from observations with the Chandra HETGS of the Seyfert I AGN NGC 4593 and Mrk 509. We discuss the photoionized outflows associated with Seyfert I AGN in terms of their absorption spectral signatures and…

Astrophysics · Physics 2007-05-23 B. McKernan , T. Yaqoob

We review recent progress in elucidating the relationship between high-energy radiation and the interstellar medium (ISM) in young supernova remnants (SNRs) with ages of $\sim$2000 yr, focusing in particular on RX J1713.7$-$3946 and RCW 86.…

High Energy Astrophysical Phenomena · Physics 2021-06-29 Hidetoshi Sano , Yasuo Fukui

We present results from a combined radio, optical, and X-ray study of the jet-associated emission features in NGC1052. We analyse the radio-optical morphology and find a good positional correlation between the radio jet and the optical…

Astrophysics · Physics 2009-11-07 M. Kadler , E. Ros , J. Kerp , H. Falcke , J. A. Zensus , R. W. Pogge , G. V. Bicknell

We present Chandra and XMM-Newton observations of the composite star-forming/Seyfert galaxy IRAS20051-1117. The X-ray imaging and spectral properties reveal the presence of an active nucleus. The Chandra image shows a strong nuclear point…

Astrophysics · Physics 2009-11-10 I. Georgantopoulos , I. Papadakis , A. Zezas , M. J. Ward

New observations are reported of J-band spectra (1.04micron -- 1.4 micron) of three Seyfert 2 galaxies, Mkn 34, Mkn 78 and NGC 5929. In each case the spectral range includes the near-infrared lines of [FeII], [PII], HeI and Pa beta. Each…

Astrophysics · Physics 2008-11-26 N. Jackson , R. Beswick

We present adaptive optics-assisted J- and K-band integral field spectroscopy of the inner 300 x 300 pc of the Seyfert 2 galaxy NGC1068. The data were obtained with the Gemini NIFS integral field unit spectrometer, which provided us with…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 X. Mazzalay , A. Rodríguez-Ardila , S. Komossa , Peter J. McGregor

We present a study of the central 2.3 kpc of NGC 5135, a nearby Luminous Infrared Galaxy (LIRG) with an AGN and circumnuclear starburst. Our main results are based on intermediate spectral resolution (~ 3000-4000) near infrared data taken…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-18 A. G. Bedregal , L. Colina , A. Alonso-Herrero , S. Arribas

We present results from a half-day observation by XMM-Newton of the nucleus of the nearby Seyfert 2 galaxy NGC 6300. The X-ray spectrum of the nucleus consists of a heavily absorbed hard component dominating the 3--10 keV band and a soft…

Young radio AGN are pivotal for our understanding of many of the still-debated aspects of AGN feedback. In this paper we present a study of the interstellar medium in the compact, peaked-spectrum radio galaxy PKSB1934-63 using X-shooter…

Astrophysics of Galaxies · Physics 2018-10-03 F. Santoro , M. Rose , R. Morganti , C. Tadhunter , T. A. Oosterloo , J. Holt