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相关论文: High redshift X-ray cooling-core cluster associate…

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X-ray cluster emission has been observed mainly in clusters with "inactive" cD galaxies (L_bol ~1E40-1E43erg/sec), which do not show signs of accretion onto a SMBH. Our recent Chandra discovery of ~100kpc scale diffuse X-ray emission…

We report the Chandra discovery of an X-ray cluster at redshift z = 1.063 associated with the Compact Steep Spectrum radio loud quasar 3C 186 (Q0740+380). Diffuse X-ray emission is detected out to ~120 kpc from the quasar and contains…

We report results of an 18 ks exposure with the ACIS instrument on Chandra of the powerful z = 0.62 radio galaxy 3C 220.1. The X-ray emission separates into cluster gas of emission-weighted kT ~ 5 keV and 0.7-12 keV luminosity (to a radius…

天体物理学 · 物理学 2009-11-06 D. M. Worrall , M. Birkinshaw , M. J. Hardcastle , C. R. Lawrence

We examine the properties of the X-ray gas in the central regions of the distant (z=0.46), X-ray luminous cluster of galaxies surrounding the powerful radio source 3C 295, using observations made with the Chandra Observatory. Between radii…

We report the first significant detection of an X-ray cluster associated with a powerful (L(bol) ~1e47 erg/sec) radio-loud quasar at high redshift (z=1.06). Diffuse X-ray emission is detected out to ~120 kpc from the CSS quasar 3C 186. A…

天体物理学 · 物理学 2007-05-23 A. Siemiginowska , C. C. Cheung , S. LaMassa , D. Burke , T. L. Aldcroft , J. Bechtold , M. Elvis , D. M. Worrall

We report the detection of extended X-ray emission around several powerful 3CR quasars with redshifts out to 0.73. The ROSAT HRI images of the quasars have been corrected for spacecraft wobble and compared with an empirical point-spread…

天体物理学 · 物理学 2009-10-31 C. S. Crawford , I. Lehmann , A. C. Fabian , M. N. Bremer , G. Hasinger

Chandra X-ray observations of the high redshift (z =1.532) radio-loud quasar 3C270.1 in 2008 February show the nucleus to have a power-law spectrum, Gamma = 1.66 +/- 0.08, typical of a radio-loud quasar, and a marginally-detected Fe Kalpha…

We present results from ASCA and ROSAT HRI observations of the powerful radio galaxy 4C+55.16 at redshift 0.24. Extended soft X-ray emission is imaged by the ROSAT HRI. The X-ray brightness profile is sharply peaked on the radio galaxy,…

天体物理学 · 物理学 2009-10-31 K. Iwasawa , S. W. Allen , A. C. Fabian , A. C. Edge , S. Ettori

We present a Chandra observation of the only low redshift, z=0.299, galaxy cluster to contain a highly luminous radio-quiet quasar, H1821+643. By simulating the quasar PSF, we subtract the quasar contribution from the cluster core and…

高能天体物理现象 · 物理学 2010-08-23 H. R. Russell , A. C. Fabian , J. S. Sanders , R. M. Johnstone , K. M. Blundell , W. N. Brandt , C. S. Crawford

We report the results from a 200 ks Chandra observation of the z=1.786 radio galaxy 3C294 and its cluster environment, increasing by tenfold our earlier observation. The diffuse emission, extending about 100 kpc around the nucleus, has a…

天体物理学 · 物理学 2009-09-17 A. C. Fabian , J. S. Sanders , C. S. Crawford , S. Ettori

A third possible explanation for the X-ray emission from the z=2.156 radio galaxy 1138-262 is thermal emission from a very dense, sub-cluster `halo', perhaps associated with the (forming) cD galaxy on a scale < 100 kpc. For instance,…

天体物理学 · 物理学 2009-10-30 C. L. Carilli , D. E. Harris , L. Pentericci , H. J. A. Rottgering , G. K. Miley , M. N. Bremer

We present a 100 ks Chandra observation studying the extended X-ray emission around the powerful z=1.04 quasar PKS1229-021. The diffuse cluster X-ray emission can be traced out to ~15 arcsec (~120 kpc) radius and there is a drop in the…

宇宙学与河外天体物理 · 物理学 2015-06-03 H. R. Russell , A. C. Fabian , G. B. Taylor , J. S. Sanders , K. M. Blundell , C. S. Crawford , R. M. Johnstone , E. Belsole

We report on the detection of a soft spatially-extended component of X-ray emission around four intermediate-redshift 3C quasars observed with Chandra: 3C254, 3C263, 3C275.1 and 3C281. The bolometric luminosity of this emission ranges over…

天体物理学 · 物理学 2009-09-17 C. S. Crawford , A. C. Fabian

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…

天体物理学 · 物理学 2009-11-06 A. C. Fabian , C. S. Crawford , S. Ettori , J. S. Sanders

We present a detailed analysis of Chandra X-ray observations of the lensing cluster of galaxies CL0024+17 at z=0.395. We found that the radial temperature profile is consistent with being isothermal out to ~600 kpc and that the average…

天体物理学 · 物理学 2009-11-10 Naomi Ota , Etienne Pointecouteau , Makoto Hattori , Kazuhisa Mitsuda

The X-ray properties of a sample of high redshift (z>0.6), massive clusters observed with XMM-Newton and Chandra are described, including two exceptional systems. One, at z=0.89, has an X-ray temperature of T=11.5 (+1.1, -0.9) keV (the…

We present Chandra X-ray Observations of the Hydra A cluster of galaxies, and we report the discovery of structure in the central 80 kpc of the cluster's X-ray-emitting gas. The most remarkable structures are depressions in the X-ray…

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…

宇宙学与河外天体物理 · 物理学 2010-08-23 J. S. Sanders , A. C. Fabian , G. B. Taylor

We present new Chandra X-ray observations of the luminous X-ray cluster, MS0451.6-0305, at z=0.5386. Spectral imaging data for the cluster are consistent with an isothermal cluster of 10.0 - 10.6 +/-1.6 keV and an Fe abundance of 0.32-0.40…

天体物理学 · 物理学 2009-11-10 Megan Donahue , Jessica A. Gaskin , Sandeep K. Patel , Marshall Joy , Doug Clowe , John P. Hughes

We report the discovery of highly distorted X-ray emission associated with the nearby cluster Zw1718.1-0108, one of whose dominant members is the powerful radio galaxy 3C353. This cluster has been missed by previous X-ray cluster surveys…

天体物理学 · 物理学 2009-10-31 K. Iwasawa , S. Ettori , A. C. Fabian , A. C. Edge , H. Ebeling
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