Deprojecting galaxy-cluster cold fronts: evidence for bulk, magnetised spiral flows
arXiv:2002.00971 · doi:10.1093/mnras/staa1251
Abstract
Tangential discontinuities known as cold fronts (CFs) are abundant in groups and clusters of galaxies (GCs). The relaxed, spiral-type CFs were initially thought to be isobaric, but a significant, -- jump in the thermal pressure was reported when deprojected CFs were stacked, interpreted as missing below the CFs (i.e. at smaller radii ) due to a locally-enhanced nonthermal pressure . We report a significant () deprojected jump in across a single sharp CF in the Centaurus cluster. Additional seven CFs are deprojected in the GCs A2029, A2142, A2204, and Centaurus, all found to be consistent (stacked: ) with similar pressure jumps. Combining our sample with high quality deprojected CFs from the literature indicates pressure jumps at significance levels ranging between and , depending on assumptions. Our nominal results are consistent with $P_{nt}\simeq (0.1\mbox{--}0.3)P_t$ just below the CF. We test different deprojection and analysis methods to confirm that our results are robust, and show that without careful deprojection, an opposite pressure trend may incorrectly be inferred. Analysing all available deprojected data, we also find: (i) a nearly constant CF contrast of density and temperature within each GC, monotonically increasing with the GC mass as ; (ii) hydrostatic mass discontinuities indicating fast bulk tangential flows below all deprojected CFs, with a mean Mach number ; and (iii) the newly deprojected CFs are consistent (stacked: ) with a metallicity drop across the CF. These findings suggest that GCs quite generally harbor extended spiral flows.
arXiv comment29 pages, 20 figures, 6 tables
References in corpus (98)
- A Universal Density Profile from Hierarchical Clustering
- The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
- Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
- The Mass Function of an X-Ray Flux-Limited Sample of Galaxy Clusters
- Triaxial Modeling of Halo Density Profiles with High-resolution N-body Simulations
- An Overview of the Performance and Scientific Results from the Chandra X-Ray Observatory (CXO)
- Shocks and cold fronts in galaxy clusters
- A very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction
- A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E0657-56
- The Shape of Dark Matter Halos: Dependence on Mass, Redshift, Radius, and Formation
- Concentration, Spin and Shape of Dark Matter Haloes: Scatter and the Dependence on Mass and Environment
- Chandra temperature profiles for a sample of nearby relaxed galaxy clusters
- Chandra Observation of Abell 2142: Survival of Dense Subcluster Cores in a Merger
- Comparing the temperatures of galaxy clusters from hydro-N-body simulations to Chandra and XMM-Newton observations
- Comparing the temperatures of galaxy clusters from hydro-N-body simulations to Chandra and XMM-Newton observations
- A moving cold front in the intergalactic medium of A3667
- Absolute measurement of the unresolved cosmic X-ray background in the 0.5-8 keV band with Chandra
- The origin of cold fronts in the cores of relaxed galaxy clusters
- The Observed Growth of Massive Galaxy Clusters II: X-ray Scaling Relations
- A deeper X-ray study of the core of the Perseus galaxy cluster: the power of sound waves and the distribution of metals and cosmic rays
- Non-hydrostatic gas in the core of the relaxed galaxy cluster A1795
- Deep inside the core of Abell 1795: the Chandra view
- Measuring the Three-Dimensional Structure of Galaxy Clusters. I. Application to a Sample of 25 Clusters
- The Redshift Evolution of LCDM Halo Parameters: Concentration, Spin, and Shape
- Probing the Dark Matter and Gas Fraction in Relaxed Galaxy Groups with X-ray observations from Chandra and XMM
- Magnetic support of the optical emission line filaments in NGC 1275
- Observational Tests of the Mass-Temperature Relation for Galaxy Clusters
- X-ray Spectroscopy of the Virgo Cluster out to the Virial Radius
- Chandra constraints on the thermal conduction in the intracluster plasma of A2142
- Spatially-resolved X-ray spectroscopy of the core of the Centaurus cluster
- A wide Chandra view of the core of the Perseus cluster
- Gas sloshing, cold front formation, and metal redistribution: the Virgo cluster as a quantitative test case
- The Complex Cooling Core of Abell 2029: Radio and X-ray Interactions
- Chandra Temperature Map of Abell 754 and Constraints on Thermal Conduction
- Witnessing the Growth of the Nearest Galaxy Cluster: Thermodynamics of the Virgo Cluster Outskirts
- Suzaku measurement of Abell 2204's intracluster gas temperature profile out to 1800 kpc
- A very deep Chandra view of metals, sloshing and feedback in the Centaurus cluster of galaxies
- Occurrence of radio minihalos in a mass-limited sample of galaxy clusters
- Shock heating of the merging galaxy cluster A521
- A New Look at Massive Clusters: weak lensing constraints on the triaxial dark matter halos of Abell 1689, Abell 1835, & Abell 2204
- A statistically-selected Chandra sample of 20 galaxy clusters -- II. Gas properties and cool-core/non-cool core bimodality
- Abell 2142 at large scales: An extreme case for sloshing?
- Some like it triaxial: the universality of dark matter halo shapes and their evolution along the cosmic time
- Shock fronts, electron-ion equilibration and ICM transport processes in the merging cluster Abell 2146
- Direct X-ray Spectral Deprojection of Galaxy Clusters
- X-ray exploration of the outskirts of the nearby Centaurus cluster using Suzaku and Chandra
- Deep Chandra Observations of the Extended Gas Sloshing Spiral in A2029
- Cold Fronts: Probes of Plasma Astrophysics in Galaxy Clusters
- Minor merger-induced cold fronts in Abell 2142 and RXJ1720.1+2638
- Shapes of clusters and groups of galaxies: Comparison of model predictions with observations
- Mass, velocity anisotropy, and pseudo phase-space density profiles of Abell 2142
- Kelvin-Helmholtz instabilities at the sloshing cold fronts in the Virgo cluster as a measure for the effective ICM viscosity
- Probing the extreme realm of AGN feedback in the massive galaxy cluster, RX J1532.9+3021
- Is there a giant Kelvin-Helmholtz instability in the sloshing cold front of the Perseus cluster?
- The Effect of Anisotropic Viscosity on Cold Fronts in Galaxy Clusters
- Chandra Observation of the Merging Cluster A168: A Late Stage in the Evolution of a Cold Front
- A cluster in a crowded environment: XMM-Newton and Chandra observations of A3558
- Metal transport by gas sloshing in M87
- Measuring the Three-Dimensional Structure of Galaxy Clusters. II. Are clusters of galaxies oblate or prolate?
- Multiple density discontinuities in the merging galaxy cluster CIZA J2242.8+5301
- Deep Chandra Observations of Edges and Bubbles in the NGC 5846 Galaxy Group
- Deep Chandra observations of NGC 1404: cluster plasma physics revealed by an infalling early-type galaxy
- Feedback through multiple outbursts in the cluster 2A 0335+096
- Deep Chandra observation and numerical studies of the nearest cluster cold front in the sky
- Gas sloshing regulates and records the evolution of the Fornax Cluster
- Dynamics and Magnetization in Galaxy Cluster Cores Traced by X-ray Cold Fronts
- Core Gas Sloshing in Abell 1644
- Gas Sloshing and Bubbles in the Galaxy Group NGC 5098
- X-ray Bright Active Galactic Nuclei in Massive Galaxy Clusters I: Number Counts and Spatial Distribution
- Galaxy Clusters: Oblate or Prolate?
- Metal distribution in sloshing galaxy clusters: the case of A496
- An azimuthally resolved study of the cold front in Abell 3667
- Radio and Deep Chandra Observations of the Disturbed Cool Core Cluster Abell 133
- A Chandra X-ray Analysis of Abell 1664: Cooling, Feedback and Star Formation in the Central Cluster Galaxy
- Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster
- The axis ratio distribution of X-ray clusters observed by XMM-Newton
- CLUMP-3D. Three dimensional lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster
- Deep Chandra Observations of Abell 2199: the Interplay between Merger-Induced Gas Motions and Nuclear Outbursts in a Cool Core Cluster
- Fields and Filaments in the Core of the Centaurus Cluster
- The merging galaxy cluster A520 --- a broken-up cool core, a dark subcluster, and an X-ray channel
- Inside a Beehive: the Multiple Merging Processes in the Galaxy Cluster Abell 2142
- Sloshing cold fronts in galaxy groups and their perturbing disk galaxies: an X-ray, Optical and Radio Case Study
- Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-ray, SZ, and Lensing Data
- Cold Fronts by Merging of Shocks
- Cold fronts and multi-temperature structures in the core of Abell 2052
- The faint end of the red sequence galaxy luminosity function: unveiling surface brightness selection effects with the CLASH clusters
- Bow shock in merging cluster A520: the edge of the radio halo and the electron-ion equilibration timescale
- SMAUG: a new technique for the deprojection of galaxy clusters
- Spiral flows in cool-core galaxy clusters
- Gas Sloshing and Radio Galaxy Dynamics in the Core of the 3C449 Group
- A Chandra Study of Radial Temperature Profiles of the Intra-Cluster Medium in 50 Galaxy Clusters
- Strong Magnetization Measured in the Cool Cores of Galaxy Clusters
- I. Analysis of candidates for interacting galaxy clusters
- Gas sloshing in Abell 2204: Constraining the properties of the magnetized intracluster medium
- A Joint Chandra and XMM-Newton View of Abell 3158: Massive Off-Centre Cool Gas Clump As A Robust Diagnostic of Merger Stage
- Metal jumps across sloshing cold fronts: the case of A496
- A Dynamically Driven, Universal Thermal Profile of Galaxy Groups and Clusters
- Cold fronts in cool core clusters
Cited by in corpus (5)
- Radio halos and relics from extended cosmic-ray ion distributions with strong diffusion in galaxy clusters
- The Merger Dynamics of the X-ray Emitting Plasma in Clusters of Galaxies
- Advection by large-scale spiral flows in galaxy clusters
- Quasi-spiral solution to the mixed intracluster medium and the universal entropy profile of galaxy clusters
- Cold fronts in galaxy clusters I: A case for the large-scale global eigen modes in unmagnetized and weakly magnetized cluster core