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Related papers: Interaction in the Bimodal Galaxy Cluster A3528

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We present the results of a redshift survey of galaxies in the A3528 complex, a chain of interacting clusters in the core of the Shapley Concentration. This complex is characterized in the X-ray band by two pairs of roughly similar…

Astrophysics · Physics 2016-08-30 S. Bardelli , E. Zucca , A. Baldi

Superclusters are the largest-scale environments where a number of galaxy clusters interact with each other through minor/major mergers and grow via accretion along cosmic filaments. We focus on the A3528 complex in the core of the Shapley…

Cosmology and Nongalactic Astrophysics · Physics 2025-02-05 G. Di Gennaro , T. Venturi , S. Giacintucci , M. Brüggen , E. Bulbul , J. Sanders , A. Liu , X. Zhang , K. Trehaeven , D. Dallacasa , P. Merluzzi , T. Pasini , S. Bardelli , G. Bernardi , O. Smirnov

As part of an extensive radio--IR--optical--X-ray study of ROSAT clusters of galaxies in the Hydra region we have observed the bimodal Abell cluster A3528, located in the core of the Shapley Supercluster (z ~ 0.053), with the Molonglo…

Astrophysics · Physics 2009-10-30 A. D. Reid , R. W. Hunstead , M. M. Pierre

We analyze the XMM dataset of the interacting cluster of galaxies Abell 3528 located westward in the core of the Shapley Supercluster, the largest concentration of mass in the nearby Universe. A3528 is formed by two interacting clumps…

Astrophysics · Physics 2009-11-10 F. Gastaldello , S. Ettori , S. Molendi , S. Bardelli , T. Venturi , E. Zucca

The Shapley Supercluster ($\langle z \rangle\approx0.048$) contains several tens of gravitationally bound clusters and groups, making it it is an ideal subject for radio studies of cluster mergers. We used new high sensitivity radio…

(abridged) We present the results of a redshift survey of intercluster galaxies in the central region of the Shapley Concentration supercluster, aimed at determining the distribution of galaxies in between obvious overdensities. Our sample…

Astrophysics · Physics 2009-10-31 S. Bardelli , E. Zucca , G. Zamorani , L. Moscardini , R. Scaramella

We present here the first results of a 22cm survey of the Shapley Concentration core. The observations were carried out with the Australia Telescope Compact Array. Our radio observations completely and uniformely cover the A3558 complex,…

Astrophysics · Physics 2016-08-30 T. Venturi , R. Morganti , S. Bardelli , D. Dallacasa , R. W. Hunstead

We present an analysis of a mosaic of ROSAT PSPC and Einstein Observatory IPC X-ray observations of 14 clusters and 2 groups of galaxies, enclosed in a sky area 15 degrees by 20 degrees centred on A3558 within the Shapley Supercluster…

Astrophysics · Physics 2015-06-24 S. Ettori , A. C. Fabian , D. A. White

We present a multi-band study of the diffuse emission in the galaxy cluster Abell 3558, located in the core of the Shapley Supercluster. Using new MeerKAT UHF-Band and uGMRT Band-3 observations, and published MeerKAT L-band and ASKAP 887…

We present a combined analysis of the BeppoSAX and ROSAT PSPC observation of the cluster of galaxies A3562, a massive member of the core of the Shapley Supercluster. With a complex and interacting structure composed from two groups of…

Astrophysics · Physics 2016-08-30 S. Ettori , S. Bardelli , S. De Grandi , S. Molendi , G. Zamorani , E. Zucca

The Shapley Concentration ($z\approx0.048$) covers several degrees in the Southern Hemisphere, and includes galaxy clusters in advanced evolutionary stage, groups of clusters in the early stages of merger, fairly massive clusters with…

We report the first results of a spectroscopic survey of galaxies in the core of the Shapley Concentration, the richest nearby supercluster of clusters of galaxies. We have measured 311 new galaxy redshifts in an area of $\sim 4.5$ square…

Astrophysics · Physics 2015-06-24 S. Bardelli , E. Zucca , G. Vettolani , G. Zamorani

The core region is dominated by three rich Abell clusters and two poor clusters. Their spatial distributions of gas temperature and metal abundance provide us with information on the interactions and motions of member clusters. From eight…

Astrophysics · Physics 2009-11-10 F. Akimoto , K. Kondou , A. Furuzawa , Y. Tawara , K. Yamashita

We investigate the dynamical properties of the cluster of galaxies A3558 (Shapley 8). Studying a region of one square degree ($\sim$ 3 Mpc$^2$) centered on the cluster cD galaxy, we have obtained a statistically complete photometric catalog…

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…

Astrophysics · Physics 2009-09-17 R. M. Johnstone , A. C. Fabian , R. G. Morris , G. B. Taylor

The core of the Shapley supercluster (A3556, A3558, SC1327-312, SC1329-313, and A3562) is an ideal region in which to study the effects of cluster mergers on the activity of individual galaxies. This paper presents the most comprehensive…

Astrophysics · Physics 2008-11-26 Neal A. Miller

We report and discuss the results of a 22 cm radio survey carried out with the Australia Telescope Compact Array (ATCA) covering the A3528 complex, a chain formed by the merging ACO clusters A3528-A3530-A3532, located in the central region…

Astrophysics · Physics 2009-11-06 T. Venturi , S. Bardelli , G. Zambelli , R. Morganti , R. W. Hunstead

Galaxy clusters produce a very hostile environment to galaxies, whose gas gets stripped by ram-pressure, suffer galaxy interactions and witness quenching of their star formation. Clusters, like Abell 2142, grow not only through galaxy…

The Shapley Concentration is the richest supercluster of clusters in the nearby universe and its core is a remarkable complex formed by the ACO clusters A3558, A3562 and A3556, and by the two minor groups SC 1327-312 and SC 1329-314. This…

Astrophysics · Physics 2009-10-30 S. Bardelli , E. Zucca , G. Zamorani , G. Vettolani , R. Scaramella

We study the radio continuum emission of four galaxies experiencing ram-pressure stripping in four clusters of the Shapley supercluster at redshift z~0.05. Multi-band (235-1367 MHz) radio data, complemented by integral-field spectroscopy,…

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