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Title: MC2: Multiwavelength and Dynamical Analysis of the Merging Galaxy Cluster ZwCl 0008.8+5215: An Older and Less Massive Bullet Cluster

Journal Article · · The Astrophysical Journal (Online)
ORCiD logo [1]; ORCiD logo [2];  [3];  [4]; ORCiD logo [5]
  1. Univ. of California, Davis, CA (United States)
  2. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  3. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  4. Univ. of California, Davis, CA (United States); Yonsei Univ., Seoul (Korea, Republic of)
  5. Univ. of California, Davis, CA (United States); Univ. de Lisboa, Lisbon (Portugal)

Here we present and analyze a rich data set including Subaru/SuprimeCam, HST/Advanced Camera for Surveys and Wide Field Camera 3, Keck/DEIMOS, Chandra/ACIS-I, and JVLA/C and D array for the merging cluster of galaxies ZwCl 0008.8+5215. With a joint Subaru+HST weak gravitational lensing analysis, we identify two dominant subclusters and estimate the masses to be $${M}_{200}={5.7}_{-1.8}^{+2.8}\times {10}^{14}\,{M}_{\odot }$$ and $${1.2}_{-0.6}^{+1.4}\times {10}^{14}\,{M}_{\odot }$$. We estimate the projected separation between the two subclusters to be $${924}_{-206}^{+243}\,\mathrm{kpc}$$. We perform a clustering analysis of spectroscopically confirmed cluster member galaxies and estimate the line-of-sight velocity difference between the two subclusters to be $$92\pm 164\,\mathrm{km}\,{{\rm{s}}}^{-1}$$. We further motivate, discuss, and analyze the merger scenario through an analysis of the 42 ks of Chandra/ACIS-I and JVLA/C and D array polarization data. The X-ray surface brightness profile reveals a merging gas-core reminiscent of the Bullet Cluster. The global X-ray luminosity in the 0.5–7.0 keV band is $$1.7\pm 0.1\times {10}^{44}\,\mathrm{erg}\,{{\rm{s}}}^{-1}$$ and the global X-ray temperature is 4.90 ± 0.13 keV. The radio relics are polarized up to $$40 \% $$, and along with the masses, velocities, and positions of the two subclusters, we input these quantities into a Monte Carlo dynamical analysis and estimate the merger velocity at pericenter to be $${1800}_{-300}^{+400}\,\mathrm{km}\,{{\rm{s}}}^{-1}$$. This is a lower-mass version of the Bullet Cluster and therefore may prove useful in testing alternative models of dark matter (DM). We do not find significant offsets between DM and galaxies, but the uncertainties are large with the current lensing data. Furthermore, in the east, the BCG is offset from other luminous cluster galaxies, which poses a puzzle for defining DM–galaxy offsets.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA)
Grant/Contract Number:
AC52-07NA27344; 1518246; HST-GO-13343.001-A; GO5-14130X; NAS8-03060
OSTI ID:
1660517
Report Number(s):
LLNL-JRNL-774223; 966886; TRN: US2203523
Journal Information:
The Astrophysical Journal (Online), Vol. 838, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 24 works
Citation information provided by
Web of Science

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Cited By (14)

Diffuse Radio Emission from Galaxy Clusters journal February 2019
Dark matter dynamics in Abell 3827: new data consistent with standard cold dark matter journal April 2018
Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-selected Sample of 29 Merging Galaxy Clusters journal February 2019
Multi-phenomena Modeling of the New Bullet-like Cluster ZwCl 008.8+52 Using N -body/Hydrodynamical Simulations journal July 2018
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers journal September 2019
Polarization of radio relics in galaxy clusters journal November 2019
Dark matter dynamics in Abell 3827: New data consistent with standard cold dark matter text January 2018
Brightest Cluster Galaxy Alignments in Merging Clusters journal March 2019
Evidence for a Merger-induced Shock Wave in ZwCl 0008.8+5215 with Chandra and Suzaku journal March 2019
Simulated Analogs of Merging Galaxy Clusters Constrain the Viewing Angle journal August 2018
Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z > 1 journal December 2019
Dynamical Properties of Merging Galaxy Clusters from Simulated Analogs journal August 2019
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers text January 2018
Brightest Cluster Galaxy Alignments in Merging Clusters text January 2018