中文
相关论文

相关论文: A Chandra X-ray Study of Cygnus A - II. The Nucleu…

200 篇论文

We report Chandra imaging-spectroscopy and RXTE spectroscopy of the nearby, powerful radio galaxy Cygnus A. Various aspects of the results are discussed, including the X-ray properties of the nucleus, the radio hot spots, the cluster of…

天体物理学 · 物理学 2007-05-23 A. S. Wilson , K. A. Arnaud , D. A. Smith , Y. Terashima , A. J. Young

We report X-ray observations of the powerful radio galaxy Cygnus A with the Chandra X-ray Observatory. This letter focuses on the radio hot spots, all four of which are detected in X-rays with a very similar morphology to their radio…

天体物理学 · 物理学 2009-10-31 A. S. Wilson , A. J. Young , P. L. Shopbell

We present X-ray spectra of the nucleus of the nearby radio galaxy Centaurus A from observations with the XMM-Newton EPIC CCD cameras (two exposures separated by 12 months) and the Chandra HETGS. For the first time in an FRI type galaxy, we…

天体物理学 · 物理学 2007-05-23 D. A. Evans , R. P. Kraft , D. M. Worrall , M. J. Hardcastle , C. Jones , W. R. Forman , S. S. Murray

We present results from the zeroth-order imaging of a Chandra HETGS observation of the nearby Seyfert 2 galaxy Circinus. Twelve X-ray sources were detected in the ACIS-S image of the galaxy, embedded in diffuse X-ray emission. The latter…

天体物理学 · 物理学 2009-10-31 R. M. Sambruna , W. N. Brandt , G. Chartas , H. Netzer , S. Kaspi , G. P. Garmire , J. A. Nousek , K. A. Weaver

We present a Chandra ACIS-S observation of the nuclear region of the nearby spiral galaxy M51 (NGC 5194), which has a low-luminosity Seyfert 2 nucleus. The X-ray image shows the nucleus, southern extranuclear cloud, and northern loop, the…

天体物理学 · 物理学 2009-11-06 Yuichi Terashima , Andrew S. Wilson

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

The results from a recent Chandra ACIS-S study of the cluster surrounding Cygnus A are presented. We have deprojected the X-ray spectra taken from various elliptical shells in order to derive the run of temperature, density, pressure, and…

天体物理学 · 物理学 2009-11-07 David A. Smith , Andrew S. Wilson , Keith A. Arnaud , Yuichi Terashima , Andrew J. Young

We report new HST WFPC2 and NICMOS observations of the center of the nearest radio galaxy Centaurus A (NGC 5128) and discuss their implications for our understanding of the active nucleus and jet. We detect the active nucleus in the near-IR…

We report X-ray observations of the nearby, powerful radio galaxy Pictor A with the Chandra Observatory and optical and near uv observations of its western radio hot spot with the Hubble Space Telescope. X-ray emission is detected from the…

天体物理学 · 物理学 2009-10-31 A. S. Wilson , A. J. Young , P. L. Shopbell

We present high angular resolution X-ray images and spectra from two {\em Chandra} ACIS-I observations of the X-ray jet in the nearby radio galaxy Centaurus A. We find that the X-ray emission from the jet is composed of a low surface…

天体物理学 · 物理学 2009-11-07 R. P. Kraft , W. R. Forman , C. Jones , S. S. Murray , M. J. Hardcastle , D. M. Worrall

We present the first results from 60ks of observations of Arp 220 using the ACIS-S instrument on Chandra. We report the detection of several sources near the galaxy's nucleus, including a point source with a hard spectrum that is coincident…

天体物理学 · 物理学 2009-11-07 D. L. Clements , J. C. McDowell , S. Shaked , A. C. Baker , K. Borne , L. Colina , S. Lamb , C. Mundell

The nearby galaxy M33 hosts the most luminous steady X-ray source in the Local Group. The high spatial resolution of Chandra allows us to confirm that this ultra-luminous X-ray source is within the nucleus and rule out at the 4.6 sigma…

天体物理学 · 物理学 2009-11-07 Guillaume Dubus , Robert E. Rutledge

Here we re-analyze the archival {\it Chandra} data for the central parts of the Centaurus\,A radio galaxy, aiming for a systematic investigation of the X-ray emission associated with the inner radio lobes in the system, and their immediate…

高能天体物理现象 · 物理学 2020-11-10 Dominika Ł. Król , Volodymyr Marchenko , Michał Ostrowski , Łukasz Stawarz

Centaurus A, at a distance of less than 4 Mpc, is the nearest radio-loud AGN. Its emission is detected from radio to very-high energy gamma-rays. Despite the fact that Cen A is one of the best studied extragalactic objects the origin of its…

高能天体物理现象 · 物理学 2015-05-14 H. Steinle

Cygnus A, the nearest truly powerful radio galaxy, resides at the centre of a massive galaxy cluster. Chandra X-ray observations reveal its cocoon shocks, radio lobe cavities and an X-ray jet, which are discussed here. It is argued that…

高能天体物理现象 · 物理学 2015-06-23 Paul E. J. Nulsen , Andrew J. Young , Ralph P. Kraft , Brian R. McNamara , Michael W. Wise

We present the first direct imaging of what may be the thick torus in the active galactic nucleus (AGN) of the archetype powerful radio galaxy Cygnus A, using the Jansky Very Large Array (VLA) at 18 GHz to 48 GHz, with a resolution down to…

高能天体物理现象 · 物理学 2019-07-17 C. L. Carilli , R. A. Perley , V. Dhawan , D. A. Perley

We examine Chandra observations of the powerful Fanaroff-Riley class II (FR II) radio galaxy Cygnus A for an X-ray counterpart to the radio transient Cygnus A-2 that was first detected in 2011. Observations are performed using the…

高能天体物理现象 · 物理学 2022-02-23 Bradford Snios , Martijn De Vries , Paul E. J. Nulsen , Ralph P. Kraft , Aneta Siemiginowska , Michael W. Wise

In this paper, we focus on the limb-brightened, prolate spheroidal cavity of the radio galaxy Cygnus A, as revealed by the Chandra X-ray Observatory. We use the shock heated, thermal intracluster medium around the expanding cavity to infer…

天体物理学 · 物理学 2009-11-11 A. S. Wilson , David A. Smith , A. J. Young

We report preliminary results from an arcsecond-resolution X-ray survey of nearby galaxies using ACIS on board Chandra. The total sample consists of 41 low-luminosity AGNs, including Seyferts, LINERs, and LINER/H II transition objects. In…

We present a 200 ks Chandra ACIS-I image of Cygnus A, and discuss a long linear feature seen in its counterlobe. This feature has a non-thermal spectrum and lies on the line connecting the brighter hotspot on the approaching side and the…

天体物理学 · 物理学 2009-06-23 K. C. Steenbrugge , K. M. Blundell , P. Duffy
‹ 上一页 1 2 3 10 下一页 ›