MC2: MAPPING the DARK MATTER DISTRIBUTION of the "tOOTHBRUSH" CLUSTER RX J0603.3+4214 with HUBBLE SPACE TELESCOPE and SUBARU WEAK LENSING

M. James Jee, William A. Dawson, Andra Stroe, David Wittman, Reinout J. Van Weeren, Marcus Brüggen, Maruša Bradač, Huub Röttgering

Research output: Contribution to journalArticle

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Abstract

The galaxy cluster RX J0603.3+4214 at z = 0.225 is one of the rarest clusters boasting an extremely large (∼2 Mpc) radio relic. Because of the remarkable morphology of the relic, the cluster is nicknamed the "Toothbrush Cluster." Although the cluster's underlying mass distribution is one of the critical pieces of information needed to reconstruct the merger scenario responsible for the puzzling radio relic morphology, its proximity to the Galactic plane b ∼ 10° has imposed significant observational challenges. We present a high-resolution weak-lensing study of the cluster with Subaru/Suprime Cam and Hubble Space Telescope imaging data. Our mass reconstruction reveals that the cluster is composed of complicated dark matter substructures closely tracing the galaxy distribution, in contrast, however, with the relatively simple binary X-ray morphology. Nevertheless, we find that the cluster mass is still dominated by the two most massive clumps aligned north-south with a ∼3:1 mass ratio ( and for the northern and southern clumps, respectively). The southern mass peak is ∼2′ offset toward the south with respect to the corresponding X-ray peak, which has a "bullet"-like morphology pointing south. Comparison of the current weak-lensing result with the X-ray, galaxy, and radio relic suggests that perhaps the dominant mechanism responsible for the observed relic may be a high-speed collision of the two most massive subclusters, although the peculiarity of the morphology necessitates involvement of additional subclusters. Careful numerical simulations should follow in order to obtain more complete understanding of the merger scenario utilizing all existing observations.

Original languageEnglish
Article number179
JournalAstrophysical Journal
Volume817
Issue number2
DOIs
Publication statusPublished - 2016 Feb 1

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radio
merger
clumps
galaxies
cams
collision
x rays
tracing
substructures
mass distribution
Hubble Space Telescope
mass ratios
proximity
dark matter
high speed
simulation
collisions
high resolution
distribution
speed

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Jee, M. James ; Dawson, William A. ; Stroe, Andra ; Wittman, David ; Van Weeren, Reinout J. ; Brüggen, Marcus ; Bradač, Maruša ; Röttgering, Huub. / MC2 : MAPPING the DARK MATTER DISTRIBUTION of the "tOOTHBRUSH" CLUSTER RX J0603.3+4214 with HUBBLE SPACE TELESCOPE and SUBARU WEAK LENSING. In: Astrophysical Journal. 2016 ; Vol. 817, No. 2.
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abstract = "The galaxy cluster RX J0603.3+4214 at z = 0.225 is one of the rarest clusters boasting an extremely large (∼2 Mpc) radio relic. Because of the remarkable morphology of the relic, the cluster is nicknamed the {"}Toothbrush Cluster.{"} Although the cluster's underlying mass distribution is one of the critical pieces of information needed to reconstruct the merger scenario responsible for the puzzling radio relic morphology, its proximity to the Galactic plane b ∼ 10° has imposed significant observational challenges. We present a high-resolution weak-lensing study of the cluster with Subaru/Suprime Cam and Hubble Space Telescope imaging data. Our mass reconstruction reveals that the cluster is composed of complicated dark matter substructures closely tracing the galaxy distribution, in contrast, however, with the relatively simple binary X-ray morphology. Nevertheless, we find that the cluster mass is still dominated by the two most massive clumps aligned north-south with a ∼3:1 mass ratio ( and for the northern and southern clumps, respectively). The southern mass peak is ∼2′ offset toward the south with respect to the corresponding X-ray peak, which has a {"}bullet{"}-like morphology pointing south. Comparison of the current weak-lensing result with the X-ray, galaxy, and radio relic suggests that perhaps the dominant mechanism responsible for the observed relic may be a high-speed collision of the two most massive subclusters, although the peculiarity of the morphology necessitates involvement of additional subclusters. Careful numerical simulations should follow in order to obtain more complete understanding of the merger scenario utilizing all existing observations.",
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MC2 : MAPPING the DARK MATTER DISTRIBUTION of the "tOOTHBRUSH" CLUSTER RX J0603.3+4214 with HUBBLE SPACE TELESCOPE and SUBARU WEAK LENSING. / Jee, M. James; Dawson, William A.; Stroe, Andra; Wittman, David; Van Weeren, Reinout J.; Brüggen, Marcus; Bradač, Maruša; Röttgering, Huub.

In: Astrophysical Journal, Vol. 817, No. 2, 179, 01.02.2016.

Research output: Contribution to journalArticle

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