King, L. J. and Clowe, D. I. and Coleman, J. E. and Russell, H.R. and Santana, R. and White, J. A. and Canning, R. E. A. and Deering, N. J. and Fabian, A.C. and Lee, B. E. and Li, B. and McNamara, B. R. (2016) 'The distribution of dark and luminous matter in the unique galaxy cluster merger Abell 2146.', Monthly notices of the Royal Astronomical Society., 459 (1). pp. 517-527.
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 Chandra X-ray Observatory, consistent with a merger close to the plane of the sky, caught soon after first core passage. A weak gravitational lensing analysis of the total gravitating mass in the system, using the distorted shapes of distant galaxies seen with ACS-WFC on Hubble Space Telescope, is presented. The highest peak in the reconstruction of the projected mass is centred on the Brightest Cluster Galaxy (BCG) in Abell 2146-A. The mass associated with Abell 2146-B is more extended. Bootstrapped noise mass reconstructions show the mass peak in Abell 2146-A to be consistently centred on the BCG. Previous work showed that BCG-A appears to lag behind an X-ray cool core; although the peak of the mass reconstruction is centred on the BCG, it is also consistent with the X-ray peak given the resolution of the weak lensing mass map. The best-fit mass model with two components centred on the BCGs yields M200 = 1.1×1015 M⊙ and 3[Math Processing Error]×1014 M⊙ for Abell 2146-A and Abell 2146-B respectively, assuming a mass concentration parameter of c = 3.5 for each cluster. From the weak lensing analysis, Abell 2146-A is the primary halo component, and the origin of the apparent discrepancy with the X-ray analysis where Abell 2146-B is the primary halo is being assessed using simulations of the merger.
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|Publisher Web site:||http://dx.doi.org/10.1093/mnras/stw507|
|Publisher statement:||This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.|
|Date accepted:||01 March 2016|
|Date deposited:||22 April 2016|
|Date of first online publication:||07 March 2016|
|Date first made open access:||22 April 2016|
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