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相关论文: Interaction of Cygnus A with its environment

200 篇论文

We present deep GALEX images of NGC 5128, the parent galaxy of Centaurus A. We detect a striking "weather ribbon" of Far-UV and H$\alpha$ emission, which extends more than 35 kpc northeast of the galaxy. The ribbon is associated with a…

星系天体物理 · 物理学 2015-06-23 Susan G. Neff , Jean A. Eilek , Frazer N. Owen

Shock heating by radio jets is potentially an important process in a range of environments, as it will increase the entropy of the heated gas. Although this process is expected to occur in the most powerful radio-loud AGN, strong shocks…

天体物理学 · 物理学 2015-06-24 J. H. Croston , R. P. Kraft , M. J. Hardcastle

We discovered an X-ray cluster in a recent pointed Chandra observation of the radio-loud compact-steep-spectrum source 1321+045 at the redshift of 0.263. 1321+045 is part of larger survey which aims to study the X-rays properties of weak…

星系天体物理 · 物理学 2013-11-18 Maciej Ceglowski , Magdalena Kunert-Bajraszewska , A. Siemiginowska , A. Labiano , M. Guainazzi

Spitzer Space Telescope mid-infrared images of the radio galaxy Centaurus A reveal a shell-like, bipolar, structure 500 pc to the north and south of the nucleus. This shell is seen in 5.8, 8.0 and 24 micron broad-band images. Such a…

Recent observations have revealed interstellar features that apparently connect energetic activity in the central region of our Galaxy to its halo. The nature of these features, however, remains largely uncertain. We present a Chandra…

高能天体物理现象 · 物理学 2021-06-02 Q. Daniel Wang

We present results from a sensitive high-resolution X-ray observation of the nearby active galaxy Centaurus A (NGC 5128) with the ROSAT HRI. The 65~ksec X-ray image clearly distinguishes different components of the X-ray emission from Cen…

天体物理学 · 物理学 2009-10-28 S. Doebereiner , N. Junkes , S. J. Wagner , H. Zinnecker , R. Fosbury , G. Fabbiano , E. J. Schreier

Results from Chandra studies of the intracluster medium around M87 and Cygnus A are summarized.

天体物理学 · 物理学 2007-05-23 Andrew S. Wilson , Andrew J. Young , David A. Smith

The physical state of the gas in the central 500 pc of NGC~5128 (the radio galaxy Centaurus A - Cen A), was investigated using the far-infrared fine-structure lines of carbon, oxygen, and nitrogen, as well as the CO(4-3) molecular line. The…

星系天体物理 · 物理学 2017-03-01 F. P. Israel , R. Guesten , R. Meijerink , M. A. Requena-Torres , J. Stutzki

We analyzed the zero-order image of a 50 ks Chandra gratings observation of Circinus X-1, taken in 2005 during the source's low-flux state. Circinus X-1 is an accreting neutron star that exhibits ultra-relativistic arcsecond-scale radio…

天体物理学 · 物理学 2009-11-13 S. Heinz , N. S. Schulz , W. N. Brandt , D. K. Galloway

We present Chandra and radio observations, and analysis of Sloan Digital Sky Survey data, of the radio galaxy B2 0838+32A (4C 32.26) and its environment. The radio galaxy is at the centre of a nearby group that has often been identified…

天体物理学 · 物理学 2009-11-13 Nazirah N. Jetha , Martin J. Hardcastle , Trevor J. Ponman , Irini Sakelliou

The Cygnus X region contains giant molecular cloud complexes and populous associates of massive young stars. The discovery of spatially extended, hard gamma-ray emission in Cygnus X by both Milagro and Fermi indicates that Cygnus X is also…

高能天体物理现象 · 物理学 2017-09-13 Tova M. Yoast-Hull , John S. Gallagher , Francis Halzen , Ali Kheirandish , Ellen G. Zweibel

The most spectacular aspect of cluster radio emission is represented by the large-scale diffuse radio sources, which cannot be obviously associated with any individual galaxy. These sources demonstrate the existence of relativistic…

天体物理学 · 物理学 2007-12-14 Luigina Feretti

We report on a recent Chandra ACIS-S observation of the Circinus galaxy. These observations confirm that the nuclear spectrum results from reflection of a hard X-ray continuum by ``neutral'' matter. The nuclear X-ray emission is extended by…

天体物理学 · 物理学 2009-11-06 David A. Smith , Andrew S. Wilson

A puzzling feature of the {\it Chandra}--detected quasar jets is that their X-ray emission decreases faster along the jet than their radio emission, resulting to an outward increasing radio to X-ray ratio. In some sources this behavior is…

天体物理学 · 物理学 2016-08-30 Markos Georganopoulos , Demosthenes Kazanas

We present Very Long Baseline Array (VLBA) HI absorption observations of the core region of the powerful radio galaxy Cygnus A. These data show both broad (FWHM = 231 \pm 21 km/s) and narrow (FWHM <30 km/s) velocity width absorption…

宇宙学与河外天体物理 · 物理学 2015-05-14 Christian Struve , John E. Conway

We use 2.0 Msec of Chandra observations to investigate the cocoon shocks of Cygnus A and some implications for its lobes and jet. Measured shock Mach numbers vary in the range 1.18-1.66 around the cocoon. We estimate a total outburst energy…

Centaurus A, the closest active galaxy, has been detected from radio to high-energy gamma-rays. The synchrotron radiation by extremely high energy protons may be a suitable mechanism to explain the MeV to GeV emission detected by the…

高能天体物理现象 · 物理学 2015-05-13 M. Orellana , G. E. Romero

The Galactic center (GC) provides a unique laboratory for a detailed examination of the interplay between massive star formation and the nuclear environment of our Galaxy. Here, we present an 100 ks Chandra ACIS observation of the Arches…

天体物理学 · 物理学 2009-11-11 Q. Daniel Wang , Hui Dong , Cornelia Lang

Compact radio cores are not only common in radio galaxies and quasars but also in many nearby galaxies with low-active, supermassive black holes. One famous example is the Galactic Center source Sgr A*. Recent studies of proper motions and…

天体物理学 · 物理学 2007-05-23 Heino Falcke

We report on a detailed spatial and spectral analysis of the large-scale X-ray emission from the merging cluster Cygnus A. We use 2.2 Ms Chandra and 40 ks XMM-Newton archival datasets to determine the thermodynamic properties of the…

宇宙学与河外天体物理 · 物理学 2024-01-08 Anwesh Majumder , M. W. Wise , A. Simionescu , M. N. de Vries