中文
相关论文

相关论文: The cluster-scale AGN outburst in Hydra A

200 篇论文

The radio source Hercules A resides at the center of a cooling flow cluster of galaxies at redshift z = 0.154. A Chandra X-ray image reveals a shock front in the intracluster medium (ICM) surrounding the radio source, about 160 kpc from the…

天体物理学 · 物理学 2009-11-11 P. E. J. Nulsen , D. C. Hambrick , B. R. McNamara , D. Rafferty , L. Birzan , M. W. Wise , L. P. David

We present the results of a Chandra study of the Hydra A galaxy cluster, where a powerful AGN outburst created a large-scale cocoon shock. We investigated possible azimuthal variations in shock strength and shape, finding indications for a…

宇宙学与河外天体物理 · 物理学 2015-05-27 Myriam Gitti , Paul E. J. Nulsen , Laurence P. David , Brian R. McNamara , Michael W. Wise

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 analyzed a deep XMM-Newton observation of the cluster of galaxies Hydra A, focusing on the large-scale shock discovered as a surface brightness discontinuity in Chandra images. The shock front can be seen both in the pressure map and in…

The radio lobes of Hydra A lie within cavities surrounded by a rim of enhanced X-ray emission in the intracluster gas. Although the bright rim appears cooler than the surrounding gas, existing Chandra data do not exclude the possibility…

天体物理学 · 物理学 2009-11-07 P. E. J. Nulsen , L. P. David , B. R. McNamara , C. Jones , W. R. Forman , M. Wise

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 results from a deep Chandra observation of Abell 2052. A2052 is a bright, nearby, cooling flow cluster, at a redshift of z=0.035. Concentric surface brightness discontinuities are revealed in the cluster center, and these…

宇宙学与河外天体物理 · 物理学 2011-02-11 E. L. Blanton , S. W. Randall , E. M. Douglass , C. L. Sarazin , T. E. Clarke , B. R. McNamara

A521 is an interacting galaxy cluster located at z=0.247, hosting a low frequency radio halo connected to an eastern radio relic. Previous Chandra observations hinted at the presence of an X-ray brightness edge at the position of the relic,…

宇宙学与河外天体物理 · 物理学 2013-02-05 H. Bourdin , P. Mazzotta , M. Markevitch , Giacintucci , G. Brunetti

We present results from deeper {\em Chandra} observations of the southwest radio lobe of Centaurus A, first described by Kraft et al. (2003). We find that the sharp X-ray surface brightness discontinuity extends around $\sim$75% of the…

We present the results of new Suzaku observations of the Coma Cluster, the X-ray brightest, nearby, merging system hosting a well studied, typical giant radio halo. It has been previously shown that, on the western side of the cluster, the…

高能天体物理现象 · 物理学 2016-01-20 Y. Uchida , A. Simionescu , T. Takahashi , N. Werner , Y. Ichinohe , S. W. Allen , O. Urban , K. Matsushita

We present a detailed Chandra, XMM-Newton, VLA and HST analysis of one of the strongest cool core clusters known, RX J1532.9+3021 (z=0.3613). Using new, deep 90 ks Chandra observations, we confirm the presence of a western X-ray cavity or…

We present a detailed analysis of jet activity in the radio galaxy 3C348 at the center of the galaxy cluster Hercules A. We use archival Chandra data to investigate the jet-driven shock front, the radio-faint X-ray cavities, the eastern…

高能天体物理现象 · 物理学 2025-01-15 F. Ubertosi , Y. Gong , P. Nulsen , J. P. Leahy , M. Gitti , B. R. McNamara , M. Gaspari , M. Singha , C. O'Dea , S. Baum

This paper presents a comprehensive analysis of 30 ks Chandra and 46.8 ks (13 Hr) 1.4 GHz GMRT radio data on the cool-core cluster RXCJ0352.9+1941 with an objective to investigate AGN activities at its core. This study confirms a pair of…

高能天体物理现象 · 物理学 2024-09-04 Satish S. Sonkamble , S. K. Kadam , Surajit Paul , M. B. Pandge , P. K. Pawar , M. K. Patil

We examine atmospheric heating by radio active galactic nuclei (AGN) in distant X-ray clusters by cross correlating clusters selected from the 400 Square Degree (400SD) X-ray Cluster survey with radio sources in the NRAO VLA Sky Survey.…

宇宙学与河外天体物理 · 物理学 2015-05-28 C. -J. Ma , B. R. McNamara , P. E. J. Nulsen , R. Schaffer , A. Vikhlinin

We present a radio and X-ray study of PKS 1353-341, the brightest cluster galaxy radio source at the center of a recent Chandra-discovered X-ray cluster. Our multi-frequency VLA images reveal an edge-brightened (FR-II), double-lobed…

星系天体物理 · 物理学 2019-05-01 C. C. Cheung , Simona Giacintucci , T. E. Clarke

We present the results from a 42 ks \chandra ACIS observation of the galaxy cluster A478. This cluster is generally considered to be highly relaxed. The \chandra image reveals, for the first time, X-ray cavities in the hot gas within the…

天体物理学 · 物理学 2009-09-17 M. Sun , C. Jones , S. S. Murray , S. W. Allen , A. C. Fabian , A. C. Edge

We present an analysis of deep Chandra X-ray observations of the galaxy cluster MS 0735.6+7421, which hosts the most energetic radio AGN known. Our analysis has revealed two cavities in its hot atmosphere with diameters of 200-240 kpc. The…

星系天体物理 · 物理学 2014-05-27 A. N. Vantyghem , B. R. McNamara , H. R. Russell , R. A. Main , P. E. J. Nulsen , M. W. Wise , H. Hoekstra , M. Gitti

The massive, hot galaxy cluster PSZ2 G286.98+32.90 (hereafter PLCKG287, z=0.383) hosts a giant radio halo and two prominent radio relics which are signs of a disturbed dynamical state. However, despite optical and radio observations…

宇宙学与河外天体物理 · 物理学 2025-05-14 M. Gitti , A. Bonafede , F. Brighenti , F. Ubertosi , M. Balboni , F. Gastaldello , A. Botteon , W. Forman , R. J. van Weeren , M. Brüggen , K. Rajpurohit , C. Jones

We present Chandra and radio observations, and analysis of Sloan Digital Sky Survey data, of the radio galaxy B2 0838+32A (4C 32.26) and its environment. The radio galaxy is at the centre of a nearby group that has often been identified…

天体物理学 · 物理学 2009-11-13 Nazirah N. Jetha , Martin J. Hardcastle , Trevor J. Ponman , Irini Sakelliou

We examine deep Chandra X-ray observations of the Centaurus cluster of galaxies, Abell 3526. Applying a gradient magnitude filter reveals a wealth of structure, from filamentary soft emission on 100pc (0.5 arcsec) scales close to the…

‹ 上一页 1 2 3 10 下一页 ›