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相关论文: ROSAT HRI observations of Centaurus A

200 篇论文

We report high resolution imaging of the nucleus of the Seyfert 1 galaxy NGC 4151 obtained with a 50 ks Chandra HRC observation. The HRC image resolves the emission on spatial scales of 0.5", ~30 pc, showing an extended X-ray morphology…

星系天体物理 · 物理学 2014-11-20 Junfeng Wang , G. Fabbiano , M. Karovska , M. Elvis , G. Risaliti , A. Zezas , C. G. Mundell

We briefly review and extend our discussion of the ROSAT detection of the extraordinarily luminous (>10^{42} erg/s) partly extended (> 30 kpc diameter) X-ray emission from the double-nucleus ultraluminous infrared galaxy NGC 6240. The ROSAT…

天体物理学 · 物理学 2007-05-23 Hartmut Schulz , Stefanie Komossa , Jochen Greiner

Centaurus A (Cen A) is a bright radio source associated with the nearby galaxy NGC 5128 where high-resolution radio observations can probe the jet at scales of less than a light-day. The South Pole Telescope (SPT) and the Atacama Pathfinder…

We discuss ROSAT HRI X-ray observations of 33 very nearby galaxies, sensitive to X-ray sources down to a luminosity of approximately 10^38 erg/s. The galaxies are selected from a complete, volume limited sample of 46 galaxies with d<7 Mpc…

天体物理学 · 物理学 2009-10-31 P. Lira , A. Lawrence , R. A. Johnson

We present high spatial resolution X-ray Chandra HRC and HST WFPC2 Halpha observations of the prototypical infrared luminous galaxy NGC6240. The central region of this system shows a remarkably complex morphology, with filaments and loops…

天体物理学 · 物理学 2009-11-07 P. Lira , M. J. Ward , A. Zezas , S. S. Murray

We report the first detection, with Chandra, of X-ray emission from the jet of the powerful narrow-line radio galaxy 3C 346. X-rays are detected from the bright radio and optical knot at which the jet apparently bends by about 70 degrees.…

天体物理学 · 物理学 2009-11-10 D. M. Worrall , M. Birkinshaw

We present a spectral and spatial analysis of the nuclear and circumnuclear X-ray emission of the prominent southern starburst/Seyfert galaxy NGC 1365. To describe the X-ray spectrum of the core source, we favour a two-component model…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Hartmut Schulz

We consider whether the hard X-ray and soft gamma-ray emission from Centaurus A is beamed radiation from the active nucleus which is Compton-scattered into our line-of-sight. We derive the spectrum and degree of polarization of scattered…

天体物理学 · 物理学 2009-10-22 J. G. Skibo , C. D. Dermer , R. L. Kinzer

We present the first clear detection of ionized Fe-K emission and absorption components in the nearby radio galaxy Centaurus A, revealed by the high-resolution XRISM/Resolve detector. In the 6.5-6.9 keV band, XRISM reveals multiple Fe XXV…

We report results from Chandra observations analyzed for evidence of variability and proper motion in the X-ray jet of Centaurus A. Using data spanning 15 years, collective proper motion of $11.3\pm3.3$ mas yr$^{-1}$, or $0.68\pm0.20c$, is…

The nearly face-on SBc galaxy M83 (NGC 5236) was observed for 25 ksec with the ROSAT PSPC. We detected 13 point-like sources in this galaxy, 10 of which were previously unknown. We measured extended X-ray radiation from almost the whole…

天体物理学 · 物理学 2007-05-23 M. Ehle , W. Pietsch , R. Beck , U. Klein

We report Chandra ACIS and quasi-simultaneous RXTE observations of the nearby, powerful radio galaxy Cygnus A, with the present paper focusing on the properties of the active nucleus. In the Chandra observation, the hard (> a few keV) X-ray…

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

We observed a nearby radio galaxy, the Centaurus A (Cen A), three times with Suzaku in 2009, and measured the wide-band X-ray spectral variability more accurately than the previous measurements. The Cen A was in the active phase in 2009,…

高能天体物理现象 · 物理学 2015-05-30 Y. Fukazawa , K. Hiragi , S. Yamazaki , M. Mizuno , K. Hayashi , K. Hayashi , S. Nishino , H. Takahashi , M. Ohno

We have made ROSAT PSPC and HRI X-ray observations to study the intracluster gas surrounding the powerful radio source Hercules A. The cluster is luminous in X-rays (L_bol = 4.8x10^37 W), and the host of the radio source is the central…

天体物理学 · 物理学 2009-11-10 Nectaria A. B. Gizani , J. P. Leahy

Two X-ray bright early type galaxies, selected for their unusually high X-ray to optical flux ratio, have been observed at high spatial resolution with the ROSAT HRI. Both sources are clearly extended (more than 250 kpc in radius), thus…

天体物理学 · 物理学 2007-05-23 G. Trinchieri , W. Pietsch

We reveal the stellar light emerging from the kiloparsec-scale, ring-like structure of the NGC5128 (Centaurus A) galaxy in unprecedented detail. We use arcsecond-scale resolution near infrared images to create a "dust-free" view of the…

EGRET has detected 67 sources associated with active galactic nuclei. With the exception of radio galaxy Cen A, all are classified as belonging to the blazar class of active galactic nuclei. The cumulative exposure from multiple EGRET…

天体物理学 · 物理学 2010-12-03 P. Sreekumar , D. L. Bertsch , R. C. Hartman , P. L. Nolan , D. J. Thompson

We combine 9 ROSAT, 9 Chandra, and 2 XMM-Newton observations of the Cen~A galaxy to obtain the X-ray light curve of 1RXH J132519.8-430312 (=CXOU J132519.9$-$430317) spanning 1990 to 2003. The source reached a peak 0.1-2.4 keV flux…

天体物理学 · 物理学 2009-11-13 Kajal K. Ghosh , Mark H. Finger , Douglas A. Swartz , Allyn F. Tennant , Kinwah Wu

We observed the nearby galaxy M~51 (NGC 5194) with BeppoSAX. The X-ray properties of the nucleus below 10 keV are almost the same as the ASCA results regarding the hard component and the neutral Fe K$\alpha$ line, but the intensity is about…

天体物理学 · 物理学 2009-11-06 Yasushi Fukazawa , Naoko Iyomoto , Aya Kubota , Yukari Matsumoto , Kazuo Makishima

We model the northern middle radio lobe of Centaurus A (NGC 5128) as a buoyant bubble of plasma deposited by an intermittently active jet. The extent of the rise of the bubble and its morphology imply that the ratio of its density to that…

天体物理学 · 物理学 2009-11-07 Curtis J. Saxton , Ralph S. Sutherland , Geoffrey V. Bicknell