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相关论文: Chandra observations of dying radio sources in gal…

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We report the recent discovery of three `dying' radio galaxies belonging to the WENSS minisurvey sample: WNB1734+6407, WNB1829+6911 and WNB1851+5707. These sources have been selected on the basis of their extremely steep broad-band radio…

天体物理学 · 物理学 2007-05-23 M. Murgia , P. Parma , H. R. de Ruiter , K. -H. Mack , R. Fanti

We present the study of five `dying' nearby radio galaxies belonging to the WENSS minisurvey and to the B2 bright catalogs: WNB1734+6407, WNB1829+6911, WNB1851+5707, B2 0120+33, and B2 1610+29. These sources have been selected on the basis…

宇宙学与河外天体物理 · 物理学 2015-05-20 M. Murgia , P. Parma , K. -H. Mack , H. R. de Ruiter , R. Fanti , F. Govoni , A. Tarchi , S. Giacintucci , M. Markevitch

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 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 an analysis of the Chandra X-ray observation of Abell 2052, including large scale properties of the cluster as well as the central region which includes the bright radio source, 3C 317. We present temperature and abundance…

天体物理学 · 物理学 2011-07-18 Elizabeth L. Blanton , Craig L. Sarazin , Brian R. McNamara

Chandra images of galaxy clusters have revealed a wealth of structure unseen by previous generations of low resolution X-ray observatories. In the cores of clusters, bright, irregular X-ray emission is now routinely seen within central…

天体物理学 · 物理学 2007-05-23 B. R. McNamara

Clusters of galaxies are excellent laboratories for studying recurring nuclear activity in galactic nuclei since their hot gaseous medium can vastly prolong the detectability of their radio lobes via better confinement. We report here a…

星系天体物理 · 物理学 2022-08-31 Sameer Salunkhe , Surajit Paul , Gopal-Krishna , Satish Sonkamble , Shubham Bhagat

We present a multiwavelength study of RXC J2014.8-2430, the most extreme cool-core cluster in the Representative $XMM-Newton$ Cluster Structure Survey (REXCESS), using $Chandra$ X-ray, Southern Astrophysical Research (SOAR) Telescope,…

We present a new Chandra X-ray observation of the intracluster medium in the galaxy cluster Abell 2443, hosting an ultra-steep spectrum radio source. The data reveal that the intracluster medium is highly disturbed. The thermal gas in the…

宇宙学与河外天体物理 · 物理学 2015-06-16 T. E. Clarke , S. W. Randall , C. L. Sarazin , E. L. Blanton , S. Giacintucci

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…

Non-thermal properties of galaxy clusters have been studied with detailed and deep radio images in comparison with X-ray data. While much progress has been made, most of the studied clusters are at a relatively low redshift (z < 0.3). We…

宇宙学与河外天体物理 · 物理学 2020-08-26 G. Giovannini , M. Cau , A. Bonafede , H. Ebeling , L. Feretti , M. Girardi , M. Gitti , F. Govoni , A. Ignesti , M. Murgia , G. B. Taylor , V. Vacca

We investigate the properties of the environment around 20 powerful radio galaxies and quasars at redshifts between 0.45 and 1. Using XMM-Newton and Chandra observations we probe the spatial distribution and the temperature of the cluster…

天体物理学 · 物理学 2009-11-13 Elena Belsole , Diana M. Worrall , Martin J. Hardcastle , Judith H. Croston

We present a study of strong cool core, highly-luminous (most with L_x > 10^(45) erg/s), clusters of galaxies in which the mean jet power of the central active galactic nucleus must be very high yet no central point X-ray source is…

宇宙学与河外天体物理 · 物理学 2015-05-19 J. Hlavacek-Larrondo , A. Fabian

We present the results of deep Chandra and XMM-Newton observations of a complex merging galaxy cluster Abell 2256 (A2256) that hosts a spectacular radio relic (RR). The temperature and metallicity maps show clear evidence of a merger…

New radio and X-ray data are reported for the rich cluster Abell 2255. The cluster radio emission is characterized by the presence of a diffuse halo source, located at the cluster center, and a more peripheral ridge of radio emission which…

天体物理学 · 物理学 2007-05-23 L. Feretti , H. Boehringer , G. Giovannini , D. Neumann

We present the results of XMM-Newton observations of three high-redshift powerful radio galaxies 3C 184, 3C 292 and 3C 322. Although none of the sources lies in as rich an X-ray-emitting environment as is seen for some powerful radio…

天体物理学 · 物理学 2007-05-23 E. Belsole , D. M. Worrall , M. J. Hardcastle , M. Birkinshaw , C. R. Lawrence

We present the results of a Chandra observation of the cooling core cluster Abell 2063. Spectral analysis shows that there is cool gas (2 keV) associated with the cluster core, which is more than a factor of 2 cooler than the outer cluster…

天体物理学 · 物理学 2008-11-26 Kalin N. Kanov , Craig L. Sarazin , Amalia K. Hicks

We present a Chandra observation of Abell 2052, a cooling flow cluster with a central cD that hosts the complex radio source 3C 317. The data reveal ``holes'' in the X-ray emission that are coincident with the radio lobes. The holes are…

天体物理学 · 物理学 2009-11-06 Elizabeth L. Blanton , Craig L. Sarazin , Brian R. McNamara , Michael W. Wise

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 discovery of spatially-extended, non-thermal-like emission components in Chandra X-ray spectra for five of a sample of seven massive, merging galaxy clusters with powerful radio halos. The emission components can be fitted by…

天体物理学 · 物理学 2015-05-13 E. T. Million , S. W. Allen
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