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相关论文: Chandra observation of the multiple merger cluster…

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We present here \chandra observations of the rich cluster of galaxies A2256. In addition to the known cool subcluster, a new structure was resolved 2$'$ east of the peak of the main cluster. Its position is roughtly at the center of a…

天体物理学 · 物理学 2009-11-06 M. Sun , S. S. Murray , M. Markevitch , A. Vikhlinin

We present results from a deep Chandra X-ray observation of a merging galaxy cluster A520. A high-resolution gas temperature map, after the subtraction of the cluster-scale emission, reveals a long trail of dense, cool clumps --- apparently…

宇宙学与河外天体物理 · 物理学 2017-07-04 Qian Wang , Maxim Markevitch , Simona Giacintucci

We present an analysis of a Chandra observation of the massive, nearby galaxy cluster Abell 2319. A sharp surface brightness discontinuity--suggested by previous, lower angular resolution X-ray imaging--is clearly visible in the ACIS image.…

天体物理学 · 物理学 2009-11-10 Timothy B. O'Hara , Joseph J. Mohr , Martin A Guerrero

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…

We present deep ($205 \rm ks$), \Chandra observations of the \ab295 binary merging cluster ($z=0.30$). In the X-ray image, the secondary component is clearly visible as a surface brightness peak, while the primary cluster has a flatter…

宇宙学与河外天体物理 · 物理学 2019-04-03 Aurelia Pascut , John P. Hughes

Abell~1142 is a low-mass galaxy cluster at low redshift containing two comparable Brightest Cluster Galaxies (BCG) resembling a scaled-down version of the Coma Cluster. Our Chandra analysis reveals an X-ray emission peak, roughly 100 kpc…

高能天体物理现象 · 物理学 2016-04-20 Yuanyuan Su , David A. Buote , Fabio Gastaldello , Reinout van Weeren

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 an 82 ksec Chandra ACIS-I observation of a large-scale hierarchical complex, which consists of various clusters/groups of galaxies and low-surface brightness X-ray emission at z = 0.247. This high-resolution {\sl Chandra}…

天体物理学 · 物理学 2009-11-10 Q. Daniel Wang , Frazer Owen , Michael Ledlow

We present Chandra X-ray observations of the dynamically complex galaxy cluster Abell 119 ($z = 0.044$). A119 is host to two NAT radio sources (0053-015 & 0053-016) whose tails are oriented parallel to each other despite orthogonally…

We present an analysis of a highly asymmetric cluster merger from a Chandra observation of Abell 85. The merger shows significant disruption of the less massive subcluster from ram pressure effects. Nevertheless, a cold core, coincident…

天体物理学 · 物理学 2009-11-07 Joshua Kempner , Craig Sarazin , Paul Ricker

We present data from a Chandra observation of the nearby cluster of galaxies Abell 576. The core of the cluster shows a significant departure from dynamical equilibrium. We show that this core gas is most likely the remnant of a merging…

天体物理学 · 物理学 2009-11-10 Joshua C. Kempner , Laurence P. David

We use Chandra data to map the gas temperature in the central region of the merging cluster A2142. The cluster is markedly nonisothermal; it appears that the central cooling flow has been disturbed but not destroyed by a merger. The X-ray…

We present a new study of the merger dynamics of Abell~1775 by analyzing the high-quality Chandra and XMM-Newton archival data. We confirm/identify an arc-shaped edge (i.e., the head) at $\sim48$~kpc west of the X-ray peak, a split cold gas…

We study the structure of the galaxy cluster Abell 523 (A523) at z=0.104 using new spectroscopic data for 132 galaxies acquired at the Telescopio Nazionale Galileo, new photometric data from the Isaac Newton Telescope, and X-ray and radio…

星系天体物理 · 物理学 2016-01-27 M. Girardi , W. Boschin , F. Gastaldello , G. Giovannini , F. Govoni , M. Murgia , R. Barrena , S. Ettori , M. Trasatti , V. Vacca

We present an analysis of a Chandra observation of Abell 2034. The cluster has multiple signatures of an ongoing merger, including a cold front and probable significant heating of the intracluster medium above its equilibrium temperature.…

天体物理学 · 物理学 2009-11-07 J. C. Kempner , C. L. Sarazin , M. Markevitch

We present data from a Chandra observation of the nearby cluster of galaxies Abell 576. The core of the cluster shows a significant departure from dynamical equilibrium. We show that this core gas is most likely the remnant of a merging…

天体物理学 · 物理学 2007-05-23 Joshua C. Kempner , Laurence P. David

We present the results of a detailed analysis of the XMM-Newton observation of the galaxy cluster Abell 3921. The X-ray morphology of the cluster is elliptical, with the centroid offset from the brightest cluster galaxy by 17 arcsec, and…

天体物理学 · 物理学 2009-11-10 E. Belsole , J-L. Sauvageot , G. W. Pratt , H. Bourdin

We present a combined X-ray and optical analysis of the cold front cluster Abell 1201 using archival Chandra, data and multi-object spectroscopy taken with the 3.9m Anglo Australian and 6.5m Multiple Mirror Telescopes. This paper represents…

天体物理学 · 物理学 2011-02-11 Matt S. Owers , Paul E. J. Nulsen , Warrick J. Couch , Maxim Markevitch , Gregory B. Poole

We present an analysis of a 41 ks Chandra observation of the merging cluster Abell 2065 with the ACIS-I detector. Previous observations with ROSAT and ASCA provided evidence for an ongoing merger, but also suggested that there were two…

天体物理学 · 物理学 2009-11-11 Marios Chatzikos , Craig L. Sarazin , Joshua C. Kempner

We present the Chandra observation of the cluster of galaxies MS 1455.0+2232. From previous ASCA and ROSAT observations, this cluster was identified as a ``relaxed'' cluster that hosts one of the most massive cooling flows detected. With…

天体物理学 · 物理学 2007-05-23 P. Mazzotta , M. Markevitch , W. R. Forman , C. Jones , A. Vikhlinin , L. VanSpeybroeck
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