Discovery of a radio relic in the low mass, merging galaxy cluster PLCK G200.9-28.2
arXiv:1708.01718 · doi:10.1093/mnras/stx2031
Abstract
Radio relics at the peripheries of galaxy clusters are tracers of the elusive cluster merger shocks. We report the discovery of a single radio relic in the galaxy cluster PLCK G200.9-28.2 (, ) using the Giant Metrewave Radio Telescope at 235 and 610 MHz and the Karl G. Jansky Very Large Array at 1500 MHz. The relic has a size of Mpc, an arc-like morphology and is located at 0.9 Mpc from the X-ray brightness peak in the cluster. The integrated spectral index of the relic is . The spectral index map between 235 and 610 MHz shows steepening from the outer to the inner edge of the relic in line with the expectation from a cluster merger shock. Under the assumption of diffusive shock acceleration, the radio spectral index implies a Mach number of for the shock. The analysis of archival XMM Newton data shows that PLCK G200.9-28.2 consists of a northern brighter sub-cluster, and a southern sub-cluster in a state of merger. This cluster has the lowest mass among the clusters hosting single radio relics. The position of the Planck Sunyaev Ze'ldovich effect in this cluster is offset by 700 kpc from the X-ray peak in the direction of the radio relic, suggests a physical origin for the offset. Such large offsets in low mass clusters can be a useful tool to select disturbed clusters and to study the state of merger.
arXiv comment10 pages, 7 figures, 4 tables. Accepted for publication in MNRAS
References in corpus (46)
- The VLA Low-frequency Sky Survey
- Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample
- Particle Acceleration on Megaparsec Scales in a Merging Galaxy Cluster
- A Catalog of Galaxy Clusters Observed by XMM-Newton
- Bow shock and radio halo in the merging cluster A520
- Halo and Relic Sources in Clusters of Galaxies
- Radio signature of cosmological structure formation shocks
- Diffusive Shock Acceleration Simulations of Radio Relics
- Giant Ringlike Radio Structures Around Galaxy Cluster Abell 3376
- Radio Halo and Relic Candidates from the Westerbork Northern Sky Survey
- Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates
- Discovery of radio halos and double-relics in distant MACS galaxy clusters: clues to the efficiency of particle acceleration
- Shock acceleration as origin of the radio relic in A521?
- The "toothbrush-relic": evidence for a coherent linear 2-Mpc scale shock wave in a massive merging galaxy cluster?
- Systematic X-ray Analysis of Radio Relic Clusters with SUZAKU
- Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources: Addendum
- A new double radio relic in PSZ1 G096.89+24.17 and a radio relic mass-luminosity relation
- Non-Thermal Electron Acceleration in Low Mach Number Collisionless Shocks. II. Firehose-Mediated Fermi Acceleration and its Dependence on Pre-Shock Conditions
- Radio continuum observations of new radio halos and relics from the NVSS and WENSS surveys
- Evolution of shocks and turbulence in major cluster mergers
- The Extended GMRT Radio Halo Survey II: Further results and analysis of the full sample
- Challenges to our understanding of radio relics: X-ray observations of the Toothbrush cluster
- Low-Frequency study of two clusters of galaxies: A2744 and A2219
- Efficiency of Nonlinear Particle Acceleration at Cosmic Structure Shocks
- Radio observations of ZwCl 2341.1+0000: a double radio relic cluster
- The Extended GMRT Radio Halo Survey I: New upper limits on radio halos and mini-halos
- Discovery of spectral curvature in the shock downstream region: CIZA J2242.8+5301
- Spectral and polarization study of the double relics in Abell 3376 using the GMRT and the VLA
- Discovery of Megaparsec-Scale, Low Surface Brightness Nonthermal Emission in Merging Galaxy Clusters using the Green Bank Telescope
- How many radio relics await discovery?
- The widest-frequency radio relic spectra: observations from 150 MHz to 30 GHz
- Discovery of the first giant double radio relic in a galaxy cluster found in the PLANCK Sunyaev-Zel'dovich cluster survey: PLCK G287.0+32.9
- High Resolution XMM-Newton Spectroscopy of the Cooling Flow Cluster A3112
- A powerful double radio relic system discovered in PSZ1 G108.18-11.53: evidence for a shock with non-uniform Mach number?
- Relativistic Electron Shock Drift Acceleration in Low Mach Number Galaxy Cluster Shocks
- The radio relic in Abell 2256: overall spectrum and implications for electron acceleration
- Planck Intermediate Results. I. Further validation of new Planck clusters with XMM-Newton
- Curved Radio Spectra of Weak Cluster Shocks
- The impact of the SZ effect on cm-wavelength (1-30 GHz) observation of galaxy cluster radio relics
- Merging Galaxy Clusters: Offset Between the Sunyaev-Zel'dovich Effect and X-ray Peaks
- Sunyaev-Zel'dovich observation of the Bullet-like cluster Abell 2146 with the Arcminute Microkelvin Imager
- Discovery of a giant radio halo in a new Planck galaxy cluster PLCKG171.9-40.7
- Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
- No Shock Across Part of a Radio Relic in the Merging Galaxy Cluster ZwCl 2341.1+0000?
- Planck Intermediate Results. IV. The XMM-Newton validation programme for new Planck galaxy clusters
- Tracing low-mass galaxy clusters with radio relics: the discovery of Abell 3527-bis
Cited by in corpus (16)
- Diffuse Radio Emission from Galaxy Clusters
- The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights
- Electron Heating in Low Mach Number Perpendicular shocks. I. Heating Mechanism
- Electron Heating in Low Mach Number Perpendicular shocks. II. Dependence on the Pre-Shock Conditions
- Twin radio relics in a near-by low-mass galaxy cluster Abell 168
- MERGHERS Pilot: MeerKAT discovery of diffuse emission in nine massive Sunyaev-Zel'dovich-selected galaxy clusters from ACT
- The unusually weak and exceptionally steep radio relic in Abell 2108
- SoUthern Cluster sCale Extended Source Survey (SUCCESS): A GMRT and MeerKAT study of nine massive galaxy clusters
- Using the polarization properties of double radio relics to probe the turbulent compression scenario
- Exploring diffuse radio emission in galaxy clusters and groups with the uGMRT and the SKA
- uGMRT detection of cluster radio emission in low-mass Planck~SZ clusters
- MeerKAT's discovery of a radio relic in the bimodal merging cluster A2384
- A new enigmatic radio relic in the low mass cluster Abell 2108
- Radio-relic and the diffuse emission trail discovered in a low mass galaxy cluster Abell 1697
- MOSS I: Double radio relics in the Saraswati supercluster
- Low frequency observations of radio relics and halos