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Related papers: Cygnus A

200 papers

We report the discovery of X-ray emission from NGC 7027, a prototypical object for the study of the formation and evolution of planetary nebulae (PNs). Observations with the Advanced CCD Imaging Spectrometer (ACIS) aboard the Chandra X-ray…

Astrophysics · Physics 2009-11-06 Joel H. Kastner , Saeqa D. Vrtilek , Noam Soker

We describe results from our initial study of the diffuse X-ray emission structures in NGC 5128 (Cen A) using the Chandra X-ray Observatory observations. The high-angular resolution Chandra images reveal multi-scale X-ray struct ures with…

Astrophysics · Physics 2009-11-07 M. Karovska , G. Fabbiano , F. Nicastro , M. Elvis , R. P. Kraft , S. S. Murray

We present results from new Chandra and archival HST and VLA imaging observations of the circumnuclear extended emission in the nearby Type 2 Seyfert galaxy NGC 2110. We find resolved soft-band X-ray emission 4'' (~160 pc) north of the…

We describe observations of the two nearest, powerful radio galaxies with the Chandra X-ray Observatory: Cygnus A (z = 0.0562) and Pictor A (z = 0.035). Since the early results from these observations are published elsewhere (Wilson, Young…

Astrophysics · Physics 2007-05-23 A. S. Wilson , A. J. Young , P. L. Shopbell

Centaurus A (Cen A) is the closest radio galaxy and a prime example of a low-luminosity active galactic nucleus (AGN), exhibiting complex emissions across the electromagnetic spectrum. The nature of its continuum emission, particularly the…

Astrophysics of Galaxies · Physics 2025-02-10 F. Marin , D. Hutsemékers , C. -Z. Jiang , R. Antonucci , P. M. Ogle , A. Bagul , C. Ramos Almeida , M. Berton

Here we present an analysis of the X-ray morphology and flux variability of the particularly bright and extended Western hotspot in the nearest powerful (FR II-type) radio galaxy, Pictor A, based on data obtained with the Chandra X-ray…

High Energy Astrophysical Phenomena · Physics 2020-11-18 R. Thimmappa , Ł. Stawarz , V. Marchenko , K. Balasubramaniam , C. C. Cheung , A. Siemiginowska

Here we present detailed analysis of the distinct X-ray emission features present within the Eastern radio lobe of the Pictor A galaxy, around the jet termination region, utilising the data obtained from the Chandra X-ray Observatory.…

High Energy Astrophysical Phenomena · Physics 2021-11-02 R. Thimmappa , Ł. Stawarz , U. Pajdosz-Śmierciak , K. Balasubramaniam , V. Marchenko

We report the discovery of spatially-extended, non-thermal-like emission components in Chandra X-ray spectra for five of a sample of seven massive, merging galaxy clusters with powerful radio halos. The emission components can be fitted by…

Astrophysics · Physics 2015-05-13 E. T. Million , S. W. Allen

We present a Chandra observation of the powerful radio galaxy 3C294 showing clear evidence for a surrounding intracluster medium. At a redshift of 1.786 this is the most distant cluster of galaxies yet detected in X-rays. The radio core is…

Astrophysics · Physics 2009-11-06 A. C. Fabian , C. S. Crawford , S. Ettori , J. S. Sanders

We present a simple model for an evolving radio galaxy, as it expands into the hot, X-ray emitting interstellar medium (ISM) of its host galaxy or similarly into the hot intracluster medium (ICM) of its host cluster. We solve the governing…

Astrophysics · Physics 2009-10-30 Sebastian Heinz , Christopher S. Reynolds , Mitchell C. Begelman

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

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

High spatial resolution spectroscopy at 8-13microns with T-ReCS on Gemini-S has revealed striking variations in the mid-infrared emission and absorption in the nucleus of the Circinus galaxy on sub-arcsecond scales. The core of Circinus is…

We compare the radio and soft X-ray brightness as a function of position within the young supernova remnant Cassiopeia A. A moderately strong correlation (r = 0.7) was found between the X-ray emission (corrected for interstellar absorption)…

Astrophysics · Physics 2009-10-28 Jonathan W. Keohane , Lawrence Rudnick , Martha C. Anderson

We examine the core of the X-ray bright galaxy cluster 2A 0335+096 using deep Chandra X-ray imaging and spatially-resolved spectroscopy, and include new radio observations. The set of around eight X-ray bright blobs in the core of the…

Cosmology and Nongalactic Astrophysics · Physics 2010-08-23 J. S. Sanders , A. C. Fabian , G. B. Taylor

We present preliminary results from a deep observation lasting almost 200 ks, of the centre of the Perseus cluster of galaxies around NGC 1275. The X-ray surface brightness of the intracluster gas beyond the inner 20 kpc, which contains the…

We analyse a 100-ks Chandra observation of the powerful radio galaxy, 4C60.07 at z=3.79. We identify extended X-ray emission with Lx~10^45 erg/s across a ~90-kpc region around the radio galaxy. The energetics of this X-ray halo and its…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 Ian Smail , B. D. Lehmer , R. J. Ivison , D. M. Alexander , R. G. Bower , J. A. Stevens , J. E. Geach , C. A. Scharf , K. E. K. Coppin , W. J. M. van Breugel , .

We identify optical emission-line features 700" (12 kpc) southwest of the nucleus of Centaurus A, roughly opposite the radio jet and well-known optical emission filaments associated with the northern radio structure. These regions are…

Astrophysics of Galaxies · Physics 2019-01-30 William C. Keel , Julie K. Banfield , Anne Medling , Susan G. Neff

We report results of one-day simultaneous multiwavelength observations of Cygnus X-2 using XMM, Chandra, the European VLBI Network and the XMM Optical Monitor. During the observations, the source did not exhibit Z-track movement, but…

High Energy Astrophysical Phenomena · Physics 2015-05-27 M. Balucinska-Church , N. S. Schulz , J. Wilms , A. Gibiec , M. Hanke , R. E. Spencer , A. Rushton , M. J. Church

We present a study of strong cool core, highly-luminous (most with L_x > 10^(45) erg/s), clusters of galaxies in which the mean jet power of the central active galactic nucleus must be very high yet no central point X-ray source is…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 J. Hlavacek-Larrondo , A. Fabian