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相关论文: A2163: Merger events in the hottest Abell galaxy c…

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Located at z = 0.203, A2163 is a rich galaxy cluster with an intra-cluster medium (ICM) that exhibits extraordinary properties, including an exceptionally high X-ray luminosity, average temperature, and a powerful and extended radio halo.…

宇宙学与河外天体物理 · 物理学 2015-05-20 H. Bourdin , M. Arnaud , P. Mazzotta , G. W. Pratt , J. -L. Sauvageot , R. Martino , S. Maurogordato , A. Cappi , C. Ferrari , C. Benoist

We present spectroscopy of 880 galaxies within a 2-degree field around the massive, merging cluster Abell 3266. This sample, which includes 704 new measurements, was combined with the existing redshifts measurements to generate a sample of…

星系天体物理 · 物理学 2017-05-03 Siamak Dehghan , Melanie Johnston-Hollitt , Matthew Colless , Rowan Miller

The cluster Abell 2163 is a merging system of several subclusters with complex dynamics. It presents exceptional X-rays properties (high temperature and luminosity), suggesting that it is a very massive cluster. Recent 2D analysis of the…

宇宙学与河外天体物理 · 物理学 2015-06-04 G. Soucail

We present a detailed spatial and dynamical analysis of the central $\sim$~2.2~\h~Mpc region of the galaxy cluster Abell~521 (z=0.247), based on 238 spectra obtained at the 3.6~m Telescope of ESO and at the CFHT. From the analysis of the…

天体物理学 · 物理学 2008-11-26 C. Ferrari , S. Maurogordato , A. Cappi , C. Benoist

We present new redshift measurements for 55 galaxies in the vicinity of the rich galaxy cluster Abell 665. When combined with results from the literature, we have good velocity measurements for a sample of 77 confirmed cluster members from…

天体物理学 · 物理学 2009-10-31 Percy L. Gomez , John P. Hughes , Mark Birkinshaw

Abell 2163 at $z \simeq 0.201$ is one of the most massive galaxy clusters known, very likely in a post-merging phase. Data from several observational windows suggest a complex mass structure with interacting subsystems, which makes the…

星系天体物理 · 物理学 2020-03-18 U. Rescigno , C. Grillo , M. Lombardi , P. Rosati , G. B. Caminha , M. Meneghetti , A. Mercurio , P. Bergamini , D. Coe

We present 371 galaxy velocities in the field of the very rich cluster Abell 2125 (z~0.25). These were determined using optical spectroscopy collected over several years from both the WIYN 3.5m telescope and NOAO Mayall 4m telescope. Prior…

In this paper we present new AAOmega spectroscopy of 254 galaxies within a 30' radius around Abell 3888. We combine these data with the existing redshifts measured in a one degree radius around the cluster and performed a substructure…

宇宙学与河外天体物理 · 物理学 2016-02-24 S. Shakouri , M. Johnston-Hollitt , S. Dehghan

We present a dynamical analysis of the merging galaxy cluster system Abell 2146 using spectroscopy obtained with the Gemini Multi-Object Spectrograph on the Gemini North telescope. As revealed by the Chandra X-ray Observatory, the system is…

We present the results of a new spectroscopic and photometric survey of the central region of the galaxy cluster A3921 (z=0.094). We detect the presence of two dominant clumps of galaxies: a main cluster centred on the BCG (A3921-A), and a…

天体物理学 · 物理学 2009-11-10 C. Ferrari , C. Benoist , S. Maurogordato , A. Cappi , E. Slezak

New Chandra X-ray data and extensive optical spectroscopy, obtained with AAOmega on the 3.9 m Anglo-Australian Telescope, are used to study the complex merger taking place in the galaxy cluster Abell 2744. Combining our spectra with data…

宇宙学与河外天体物理 · 物理学 2015-05-20 Matt S. Owers , Scott W. Randall , Paul E. J. Nulsen , Warrick J. Couch , Laurence P. David , Joshua C. Kempner

Abell 2146 ($z$ = 0.232) consists of two galaxy clusters undergoing a major merger. The system was discovered in previous work, where two large shock fronts were detected using the $\textit{Chandra X-ray Observatory}$, consistent with a…

We report on the detection of dark matter in the cluster of galaxies Abell~2163 using the weak gravitational distortion of background galaxies, and an analysis of the cluster X-ray emission. We find that while the qualitative distributions…

天体物理学 · 物理学 2009-10-28 G. Squires , D. M. Neumann , N. Kaiser , M. Arnaud , A. Babul , H. Böhringer , G. Fahlman , D. Woods

Abell 3266 is one of the X-ray brightest galaxy clusters in the sky and is a well-known merging system. Using the ability of the eROSITA telescope onboard SRG (Spectrum R\"ontgen Gamma) to observe a wide field with a single pointing, we…

We present a weak-lensing and dynamical study of the complex cluster Abell 1758 (A1758, z = 0.278) supported by hydrodynamical simulations. This cluster is composed of two main structures, called A1758N and A1758S. The Northern structure is…

The galaxy cluster Abell 3733 (A3733) is a very suitable candidate in addressing dynamical processes throughout galaxy cluster mergers. This study shows structural analysis results of A3733 (z = 0.038) based on X-ray and optical data.…

宇宙学与河外天体物理 · 物理学 2019-04-01 H. İ. Kaya , Turgay Caglar , Hakan Sert

We present a weak-lensing analysis of the merging cluster A2163 using Subaru/Suprime-Cam and CFHT/Mega-Cam data and discuss the dynamics of this cluster merger, based on complementary weak-lensing, X-ray, and optical spectroscopic datasets.…

宇宙学与河外天体物理 · 物理学 2015-05-28 Nobuhiro Okabe , Herve Bourdin , Pasquale Mazzotta , Sophie Maurogordato

We present a detailed strong lensing, weak lensing and X-ray analysis of Abell 2744 (z = 0.308), one of the most actively merging galaxy clusters known. It appears to have unleashed `dark', `ghost', `bullet' and `stripped' substructures,…

The mechanisms giving rise to diffuse radio emission in galaxy clusters, and in particular their connection with cluster mergers, are still debated. We aim to obtain new insights into the internal dynamics of the cluster Abell 2294,…

宇宙学与河外天体物理 · 物理学 2015-05-18 M. Girardi , W. Boschin , R. Barrena

We present the results from Suzaku observations of the hottest Abell galaxy cluster A2163 at $z=0.2$. To study the physics of gas heating in cluster mergers, we investigated hard X-ray emission from the merging cluster A2163, which hosts…

高能天体物理现象 · 物理学 2015-06-18 N. Ota , K. Nagayoshi , G. W. Pratt , T. Kitayama , T. Oshima , T. H. Reiprich
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