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We discovered an X-ray cluster in a Chandra observation of the compact steep spectrum (CSS) radio source 1321+045 (z=0.263). CSS sources are thought to be young radio objects at the beginning of their evolution and can potentially test the…

宇宙学与河外天体物理 · 物理学 2015-06-16 M. Kunert-Bajraszewska , A. Siemiginowska , A. Labiano

We present results from an analysis of a Chandra observation of the cluster of galaxies Abell 3581. We discover the presence of a point-source in the central dominant galaxy which is coincident with the core of the radio source PKS…

天体物理学 · 物理学 2009-09-17 R. M. Johnstone , A. C. Fabian , R. G. Morris , G. B. Taylor

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

We present the results of a {\it Chandra} observation of the central region of Abell 3112. This cluster has a powerful radio source in the center and was believed to have a strong cooling flow. The X-ray image shows that the intracluster…

天体物理学 · 物理学 2009-11-07 Motokazu Takizawa , Craig L. Sarazin , Elizabeth L. Blanton , Greg B. Taylor

We present a Chandra observation of the central (r< 200kpc) region of the cluster of galaxies 2A 0335+096, rich in interesting phenomena. On large scales (r> 40kpc), the X-ray surface brightness is symmetric and slightly elliptical. The…

天体物理学 · 物理学 2009-11-07 Pasquale Mazzotta , Alastair Edge , Maxim Markevitch

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…

The radio galaxy 1321+045 is a rare example of a young, compact steep spectrum source located in the center of a z=0.263 galaxy cluster. Using a combination of Chandra, VLBA, VLA, MERLIN and IRAM 30m observations, we investigate the…

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 report the analysis of the Chandra observation of XDCP J0044.0-2033, a massive, distant (z=1.579) galaxy cluster discovered in the XDCP survey. The total exposure time of 380 ks with Chandra ACIS-S provides the deepest X-ray observation…

宇宙学与河外天体物理 · 物理学 2015-06-23 P. Tozzi , J. S. Santos , M. J. Jee , R. Fassbender , P. Rosati , A. Nastasi , W. Forman , B. Sartoris , S. Borgani , H. Boehringer , B. Altieri , G. W. Pratt , M. Nonino , C. Jones

We present Chandra observations of the X-ray environment of a sample of 6 BL Lacertae objects. The improved sensitivity of the ACIS experiment allows us to separate the core X-ray emission from the contribution of diffuse emission from the…

天体物理学 · 物理学 2009-11-07 D. Donato , M. Gliozzi , R. M. Sambruna , J. E. Pesce

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 the results of two (101 ks total) Chandra observations of the z=0.778 optically selected lensing cluster RCS022434-0002.5, along with weak lensing and dynamical analyses of this object. An X-ray spectrum extracted within R(2500)…

We report the detection of the lens cluster of the gravitational lens (GL) system Q0957+561 from a deep observation with the Advanced CCD Imaging Spectrometer on-board the Chandra X-ray Observatory. Intracluster X-ray emission is found to…

天体物理学 · 物理学 2009-11-07 G. Chartas , V. Gupta , G. Garmire , C. Jones , E. E. Falco , I. I. Shapiro , F. Tavecchio

Using the deepest (370 ksec) Chandra observation of a high-redshift galaxy cluster, we perform a detailed characterization of the intra-cluster medium (ICM) of WARPJ1415.1+3612 at z=1.03. We also explore the connection between the ICM core…

宇宙学与河外天体物理 · 物理学 2015-06-03 Joana S. Santos , Paolo Tozzi , Piero Rosati , Mario Nonino , Gabriele Giovannini

We present the analysis of 30 ksec of Chandra observations of the galaxy cluster Abell 1835. Overall, the X-ray image shows a relaxed morphology, although we detect substructure in in the inner 30 kpc radius. Spectral analysis shows a steep…

天体物理学 · 物理学 2009-09-17 R. W. Schmidt , S. W. Allen , A. C. Fabian

We present results from an analysis of two Chandra observations of the rich, nearby galaxy cluster Abell 2199. We find evidence (having corrected for projection effects) for radial gradients in temperature and metallicity in the X-ray…

天体物理学 · 物理学 2009-09-17 R. M. Johnstone , S. W. Allen , A. C. Fabian , J. S. Sanders

We present the X-ray analysis and the mass estimation of the lensing cluster of galaxies CL0024+17 with Chandra. We found that the temperature profile is consistent with being isothermal and the average X-ray temperature is 4.47 (+0.83,…

天体物理学 · 物理学 2007-05-23 Naomi Ota , Makoto Hattori , Etienne Pointecouteau , Kazuhisa Mitsuda

We observed MS 1054-0321, the highest redshift cluster of galaxies in the Einstein Medium Sensitivity Survey (EMSS), with the Chandra ACIS-S detector. We find the X-ray temperature of the cluster to be 10.4 +1.7 -1.5 keV, lower than, but…

We present a Chandra observation of the cooling flow cluster Abell 262. Spectral fits show that the intracluster medium (ICM) in A262 cools by a factor of three from 2.7 keV to 0.9 keV at the cluster center. A mass deposition rate of Mdot =…

天体物理学 · 物理学 2009-11-10 Elizabeth L. Blanton , Craig L. Sarazin , Brian R. McNamara , T. E. Clarke

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
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