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相关论文: Multiple merging in the Abell cluster 1367

200 篇论文

The June 2004 version of our compilation of measured redshifts for clusters in the Abell-ACO catalogue lists redshifts for 3715 clusters/subclusters in 3033 distinct (2396 A- and 637 S-) clusters, 67% of these with N_z>=3 galaxies measured.…

天体物理学 · 物理学 2007-05-23 H. Andernach , E. Tago , M. Einasto , J. Einasto , J. Jaaniste

Using the CLASH-VLT survey, we assembled an unprecedented sample of 1234 spectroscopically confirmed members in Abell~S1063, finding a dynamically complex structure at z_cl=0.3457 with a velocity dispersion \sigma_v=1380 -32 +26 km s^-1. We…

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

We present an analysis of the structures and dynamics of the merging cluster Abell~1201, which has two sloshing cold fronts around a cooling core, and an offset gas core approximately 500kpc northwest of the center. New Chandra and…

宇宙学与河外天体物理 · 物理学 2015-06-05 Cheng-Jiun Ma , Matt Owers , Paul E. J. Nulsen , Brian R. McNamara , Stephen S. Murray , Warrick J. Couch

We report the discovery of a binary galaxy cluster merger via a search of the redMaPPer optical cluster catalog, with a projected separation of 535 kpc between the BCGs. Archival XMM-Newton spectro-imaging reveals a gas peak between the…

宇宙学与河外天体物理 · 物理学 2023-08-01 David Wittman , Rodrigo Stancioli , Kyle Finner , Faik Bouhrik , Reinout van Weeren , Andrea Botteon

The results from Suzaku observations of the galaxy cluster Abell2256 are presented. This cluster is a prototypical and well-studied merging system, exhibiting substructures both in the X-ray surface brightness and in the radial velocity…

宇宙学与河外天体物理 · 物理学 2015-05-27 Takayuki Tamura , Kiyoshi Hayashida , Shutaro Ueda , Masaaki Nagai

We present results of the X-ray analyses of the nearby cluster of galaxies Abell 2399 ($z=0.058$) using the XMM-Newton and Suzaku satellites. This cluster is classified as a low surface brightness (LSB) cluster. It has a bimodal structure…

高能天体物理现象 · 物理学 2018-11-28 Ikuyuki Mitsuishi , Yasunori Babazaki , Naomi Ota , Shin Sasaki , Hans Bohringer , Gayoung Chon , Gabriel W. Pratt

Abell 1995 is a puzzling galaxy cluster hosting a powerful radio halo, but it has not yet been recognized as a obvious cluster merger, as usually expected for clusters with diffuse radio emission. We aim at an exhaustive analysis of the…

宇宙学与河外天体物理 · 物理学 2015-06-11 W. Boschin , M. Girardi , R. Barrena

The galaxy cluster A3667 was observed using the Two-degree Field (2dF) multifibre spectroscopic system on the Anglo-Australian Telescope in a program designed to examine the velocity structure in the region. Specifically, we sought evidence…

天体物理学 · 物理学 2009-11-13 M. Johnston-Hollitt , R. W. Hunstead , E. Corbett

Based on HST and MUSE data, we probe the stellar and gas properties (i.e. kinematics, stellar mass, star formation rate) of the radio-loud brightest cluster galaxy (BCG) located at the centre of the X-ray luminous cool core cluster Abell…

We present the results of a dynamical analysis of the rich X-Ray luminous galaxy cluster Abell 521, and discuss the nature of the arc-like structure first noted by Maurogordato et al. (1996). Our study is based on radial velocities for 41…

天体物理学 · 物理学 2007-05-23 S. Maurogordato , D. Proust , T. C. Beers , M. Arnaud , R. Pello , A. Cappi , E. Slezak , J. Kriessler

We present the results of a dynamical analysis of three rich, X-ray luminous galaxy clusters, Abell 222, Abell 223 and Abell 520, that are at intermediate redshifts. Our study is based on radial velocities for 71 cluster members,…

天体物理学 · 物理学 2007-05-23 D. Proust , H. Cuevas , H. V. Capelato , L. Sodre , B. Tome Lehodey , O. Le Fevre , A. Mazure , .

We present here new insights about the merging galaxy cluster Abell 2034 ($\bar{z}=0.114$) based on a combined weak lensing and dynamical analysis. From our deep Subaru $BR_Cz'$ images plus Gemini-GMOS/N low-resolution spectra accompanied…

We describe the properties of a remarkable group of actively star-forming dwarf galaxies and HII galaxies in the Abell 1367 cluster, which were discovered in a large-scale H-alpha imaging survey of the cluster. Approximately 30…

天体物理学 · 物理学 2009-11-07 Shoko Sakai , Robert Kennicutt , J. M. van der Hulst , Chris Moss

We present a dynamical analysis of the galaxy cluster Abell 1942 based on a set of 128 velocities obtained at the European Southern Observatory. Data on individual galaxies are presented and the accuracy of the determined velocities is…

天体物理学 · 物理学 2009-11-13 H. V. Capelato , D. Proust , G. B. LIma Neto , W. A. Santos , L. Sodre

We present a catalogue of velocities for 551 galaxies (and give the coordinates of 39 stars misclassified as galaxies in our photometric plate catalogue) in a region covering about 100'$\times$100' (0.94$\times$0.94 Mpc for an average…

天体物理学 · 物理学 2009-10-30 F. Durret , P. Felenbok , C. Lobo , E. Slezak

We analyze photometric properties of 1384 cluster galaxies as a function of the normalized distance to cluster center. These galaxies were selected in the central region ($r/r_{200} \leq$ 0.8) of 14 southern Abell clusters chosen from the…

天体物理学 · 物理学 2009-11-11 V. Coenda , H. Muriel , C. J. Donzelli , H. Quintana , L. Infante , D. G. Lambas

We present new radial velocities for 306 bright (R<16) galaxies in a 77 square deg region of the Shapley supercluster measured with the FLAIR-II spectrograph on the UK Schmidt Telescope. The galaxies we measured were uniformly distributed…

天体物理学 · 物理学 2007-05-23 M. J. Drinkwater , D. Proust , Q. A. Parker , H. Quintana , E. Slezak

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…

We study luminosity and morphology segregation of over 3000 cluster galaxies in an ensemble cluster of 59 rich, nearby galaxy clusters observed in the ESO Nearby Cluster Survey (ENACS). Within this sample we identify those galaxies that are…

天体物理学 · 物理学 2009-11-07 A. Biviano , P. Katgert , T. Thomas , C. Adami