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

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We report results from our deep Chandra X-ray observations of a nearby radio galaxy, 4C+29.30 (z=0.0647). The Chandra image resolves structures on sub-arcsec to arcsec scales, revealing complex X-ray morphology and detecting the main radio…

High resolution MERLIN 5 GHz observations (0.04") of 7 Seyfert galaxies, selected as the ones previously showing evidence of collimated ejection, have been compared with high resolution archive HST data. The radio maps reveal rich…

Astrophysics · Physics 2009-11-11 E. Xanthopoulos , A. H. Thean , A. Pedlar , A. M. S. Richards

Charge exchange (CX) emission reveals the significant interaction between neutral and ionized interstellar medium (ISM) components of the dense, multiphase, circumnuclear region of a galaxy. We use a model including a thermal and a CX…

Astrophysics of Galaxies · Physics 2020-05-06 Hang Yang , Shuinai Zhang , Li Ji

High resolution spectroscopic observations of Seyfert galaxies with Chandra and XMM-Newton allows us to study the detailed ionization and thermal structures of the X-ray absorbing/emitting material in the circumnuclear environment. The vast…

We report the analysis of deep radio observations of the interacting galaxy system M51 from the Very Large Array, with the goal of understanding the nature of the population of compact radio sources in nearby spiral galaxies. We detect 107…

Astrophysics · Physics 2008-11-26 L. A. Maddox , J. J. Cowan , R. E. Kilgard , E. Schinnerer , C. J. Stockdale

Nonthermal emission observed in galaxy clusters provides a direct probe into the plasma physics of the intra-cluster medium (ICM) under extreme conditions. We report the first detailed analysis of the giant radio halo in the merging galaxy…

Cosmology and Nongalactic Astrophysics · Physics 2025-12-01 Ramananda Santra , Ruta Kale , Simona Giacintucci , Herve Bourdin , Rashi Jain , Andrea Botteon , Gianfranco Brunetti

We present the first high-resolution, soft-X-ray spectrum of the prototypical Seyfert 2 galaxy, NGC 1068. This spectrum was obtained with the XMM-Newton Reflection Grating Spectrometer. Emission lines from H-like and He-like low-Z ions…

After exploring the infrared softness diagram to characterize the hardness of the incident ionizing radiation in star-forming regions, we exploit the availability of high-excitation lines in the same spectral regime to explore its use for…

Astrophysics of Galaxies · Physics 2025-04-30 E. Pérez-Montero , J. A. Fernández-Ontiveros , B. Pérez-Díaz , J. M. Vílchez , R. Amorín

We have obtained a high spatial resolution X-ray image of the nucleus of NGC 1068 using the High Resolution Camera (HRC-I) on board the Chandra X-ray Observatory, which provides an unprecedented view of the innermost 1 arcsecond radius…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Junfeng Wang , Giuseppina Fabbiano , Margarita Karovska , Martin Elvis , Guido Risaliti

The nature of the extended hard X-ray source XMMU J061804.3+222732 and its surroundings is investigated using XMM-Newton, Chandra, and Spitzer observations. This source is located in an interaction region of the IC 443 supernova remnant…

We present James Webb Space Telescope (JWST) NIRCam imaging of the nearby Seyfert 1.9 galaxy NGC 4258, which hosts strong star formation regions as well as an anomalous jet-like radio structure that extends through a significant portion of…

Astrophysics of Galaxies · Physics 2025-08-18 Travis C. Fischer , Nicholas F. Cothard , Omnarayani Nayak , Henrique Schmitt , Erin Smith , Jason Glenn

This paper is the third in a series in which we present deep Chandra ACIS-S imaging spectroscopy of the Seyfert 1 galaxy NGC 4151, devoted to study its complex circum-nuclear X-ray emission. Emission features in the soft X-ray spectrum of…

Recent deep Chandra observations of nearby Compton thick (CT) AGN have produced surprising results, uncovering extended emission not only in the soft X-rays but in the hard emission (>3 keV), challenging the long-held belief that the…

Astrophysics of Galaxies · Physics 2023-06-28 Anna Trindade Falcao , G. Fabbiano , M. Elvis , A. Paggi , W. P. Maksym

We use the results of relativistic hydrodynamic simulations of jet-ISM interactions in a galaxy with a radio-loud AGN to quantify the extent of ionization in the central few kpcs of the gaseous galactic disc. We perform post-process…

We present a sample of 8 Seyfert 2 galaxies observed by HST, Chandra and XMM-Newton. All of the sources present soft X-ray emission which is coincident in extension and overall morphology with the [OIII] emission. The spectral analysis…

Astrophysics · Physics 2007-05-23 Stefano Bianchi , Matteo Guainazzi , Marco Chiaberge

We present a multiwavelength study of the nucleus, environment, jets, and hotspots of the nearby FRII radio galaxy 3C 321, using new and archival data from MERLIN, the VLA, Spitzer, HST, and Chandra. An initially collimated radio jet…

In this paper we discuss the X-ray properties of 49 local (z<0.035) Seyfert 2 galaxies with HST/WFC2 high-resolution optical coverage. It includes the results of 26 still unpublished Chandra and XMM-Newton observations, which yield 25 (22)…

Astrophysics · Physics 2009-11-11 M. Guainazzi , G. Matt , G. C. Perola

We investigate the physical properties of the interstellar medium (ISM) in the merging pair of galaxies known as The Antennae (NGC 4038/39), using the deep coadded ~411 ks Chandra ACIS-S data set. The method of analysis and some of the main…

Astrophysics · Physics 2009-11-13 A. Baldi , J. C. Raymond , G. Fabbiano , A. Zezas , A. H. Rots , F. Schweizer , A. R. King , T. J. Ponman

We discuss the results of a campaign to monitor spectral variations in the low-luminosity Seyfert~1 galaxy NGC~4593, at X-rays, ultraviolet, optical and near IR frequencies. The observations and data analysis have been described in a…

Astrophysics · Physics 2015-06-24 M. Santos-Lleo , J. Clavel , P. Barr , I. S. Glass , D. Pelat , B. M. Peterson , G. Reichert

XMM-Newton and Chandra/HETG spectra of the Compton-thin (NH 4x10^{23} cm^{-2}) Seyfert 2 galaxy, NGC 4507, are analyzed and discussed. The main results are: a) the soft X-ray emission is rich in emission lines; an (at least) two--zone…

Astrophysics · Physics 2009-11-10 Giorgio Matt , Stefano Bianchi , Filippo D'Ammando , Andrea Martocchia