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

Nathan Golovich, Reinout J.Van Weeren, William A. Dawson, M. James Jee, David Wittman

Research output: Contribution to journalArticle

12 Citations (Scopus)

Abstract

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 M200 = 5.7+2.8 -1.8 × 1014 M and 1.2 +1.4 -0.6 × 1014 M. We estimate the projected separation between the two subclusters to be 924+243-206kpc. 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 ± 164 kms-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 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+400-300 kms-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.

Original languageEnglish
Article number110
JournalAstrophysical Journal
Volume838
Issue number2
DOIs
Publication statusPublished - 2017 Apr 1

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galaxies
merger
dark matter
Monte Carlo analysis
estimates
cameras
polarization
x rays
radio
line of sight
brightness
gas
luminosity
analysis
temperature
profiles
gases

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

@article{601790ad2e0740779ca8ac642d32f9c8,
title = "MC2: Multiwavelength and Dynamical Analysis of the Merging Galaxy Cluster ZwCl 0008.8+5215: An Older and Less Massive Bullet Cluster",
abstract = "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 M200 = 5.7+2.8 -1.8 × 1014 M⊙ and 1.2 +1.4 -0.6 × 1014 M⊙. We estimate the projected separation between the two subclusters to be 924+243-206kpc. 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 ± 164 kms-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 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+400-300 kms-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.",
author = "Nathan Golovich and Weeren, {Reinout J.Van} and Dawson, {William A.} and Jee, {M. James} and David Wittman",
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MC2 : Multiwavelength and Dynamical Analysis of the Merging Galaxy Cluster ZwCl 0008.8+5215: An Older and Less Massive Bullet Cluster. / Golovich, Nathan; Weeren, Reinout J.Van; Dawson, William A.; Jee, M. James; Wittman, David.

In: Astrophysical Journal, Vol. 838, No. 2, 110, 01.04.2017.

Research output: Contribution to journalArticle

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