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Optical and X-Ray Observations of the Merging Cluster AS1063

Gómez, P. L. and Valkonen, L. E. and Romer, A. K. and Lloyd-Davies, E. and Verdugo, T. and Cantalupo, C. M. and Daub, M. D. and Goldstein, J. H. and Kuo, C. L. and Lange, A. E. and Lueker, M. and Holzapfel, W. L. and Peterson, J. B. and Ruhl, J. and Runyan, M. C. and Reichardt, C. L. and Sabirli, K. (2012) Optical and X-Ray Observations of the Merging Cluster AS1063. Astronomical Journal, 144 (3). Art. No. 79. ISSN 0004-6256. https://resolver.caltech.edu/CaltechAUTHORS:20120928-151230862

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Abstract

We present the first in-depth analysis of the massive cluster AS1063. This is one of the hottest X-ray clusters discovered to date and is undergoing a major merging event. The average temperature of the hot intracluster medium has been measured, using Chandra/ACIS-I, and found to be >11.5 keV. Optical spectroscopy, from GMOS-S, has provided a mean redshift of 0.3461 and a large velocity dispersion of 1840^(+230)_(–150) km s^(–1). Both the large velocity dispersion and high X-ray temperature suggest a very massive cluster (M_(200) > 2.5 × 10^(15) M_☉) and/or a merger system. The merger model is supported by a small offset between the galaxy density and the peak of the X-ray emission, the presence of offset and twisted X-ray isophotes, and a non-Gaussian galaxy velocity distribution. We also report that the velocity distribution is better represented by the velocity dispersion produced during a merger than by the velocity distribution of a relaxed cluster. Moreover, we find that two non-concentric beta models are a better description for the distribution of the cluster gas than a single beta model. Therefore, we propose that a recent merger event close to the plane of the sky is responsible for the observed properties of the cluster. In addition, optical imaging, from SuSI2 on the New Technology Telescope and GMOS-S at Gemini, has also uncovered the presence of several gravitational arcs that have been used to further constrain the mass and dynamics of the cluster.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-6256/144/3/79DOIUNSPECIFIED
http://iopscience.iop.org/1538-3881/144/3/79/PublisherUNSPECIFIED
Additional Information:© 2012 American Astronomical Society. Received 2012 April 12; accepted 2012 June 28; published 2012 August 9. This research was possible with financial support from: (1) NASA (via the XMM and Chandra Guest Observer programs and the Long Term Space Astrophysics program, grant Nos. NAG5-7926, NAG5-12999, NAG5-20453, GO4-5141X); (2) the European Commission (via a Marie Curie Reintegration Grant, grant number EIF-OIF-IIF-IRG-ERG; Project 513676); (3) AAS (via international travel grants for 2003 and 2004 and a small research grant); (4) STFC (the UK Science and Technology Facilities Council) (K.R., P.G.); (5) the Osk. Huttunen Foundation for a PhD studentship (L.V.); (6) the Magnus Ehrnrooth Foundation for a travel grant (L.V.); and (7) the University of Sussex Physics and Astronomy Department for a Graduate Teaching Assistantship (L.V.). In addition P.L.G. thanks the kindness of the Sussex Astronomy Centre during month long visits in 2006 and 2007. P.L.G. also thanks the European Southern Observatory (ESO) for two short stays at their Headquarters in Santiago where a large fraction of the final version of this paper was written. Finally, we thank the referees for helping us write a more concise, accurate, and hopefully interesting paper. This work is based on observations obtained from (1) the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Science and Technology Facilities Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministrio da Cincia e Tecnologia (Brazil), and SECYT (Argentina); (2) the Chandra X-Ray Observatory (Chandra) is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060; and (3) the ESO telescopes at La Silla under program 70.A-0074.
Funders:
Funding AgencyGrant Number
NASANAG5-7926
NASANAG5-12999
NASANAG5-20453
NASAGO4-5141X
European Commission Marie-Curie Reintegration GrantEIF-OIF-IIF-IRG-ERG 513676
AASUNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
Osk. Huttunen FoundationUNSPECIFIED
Magnus Ehrnrooth FoundationUNSPECIFIED
University of Sussex Physics and Astronomy DepartmentUNSPECIFIED
NASANAS8-03060
ESO Telescopes70.A-0074
Subject Keywords:galaxies: clusters: general
Issue or Number:3
Record Number:CaltechAUTHORS:20120928-151230862
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20120928-151230862
Official Citation:Optical and X-Ray Observations of the Merging Cluster AS1063 P. L. Gómez et al. 2012 The Astronomical Journal 144 79
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34552
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:28 Sep 2012 23:03
Last Modified:03 Oct 2019 04:20

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