The interaction between rising bubbles and cold fronts in cool core clusters
arXiv:2106.03662 · doi:10.1093/mnras/stab3655
Abstract
We investigate whether the swirling cold front in the core of the Perseus Cluster of galaxies has affected the outer buoyant bubbles that originated from jets from the Active Galactic Nucleus in the central galaxy NGC1275. The inner bubbles and the Outer Southern bubble lie along a North-South axis through the nucleus, whereas the Outer Northern bubble appears rotated about 45 deg from that axis. Detailed numerical simulations of the interaction indicates that the Outer Northern bubble may have been pushed clockwise accounting for its current location. Given the common occurrence of cold fronts in cool core clusters, we raise the possibility that the lack of many clear outer bubbles in such environments may be due to their disruption by cold fronts.
arXiv comment18 Pages, 17 Figures, submitted to MNRAS
References in corpus (48)
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- Heating Hot Atmospheres with Active Galactic Nuclei
- First results from the IllustrisTNG simulations: radio haloes and magnetic fields
- A very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction
- Chandra imaging of the complex X-ray core of the Perseus cluster
- A deep Chandra observation of the Perseus cluster: shocks and ripples
- The Quiescent Intracluster Medium in the Core of the Perseus Cluster
- The origin of cold fronts in the cores of relaxed galaxy clusters
- Simulations of magnetic fields in isolated disk galaxies
- Filaments, Bubbles, and Weak Shocks in the Gaseous Atmosphere of M87
- On the Nature of the NGC 1275 System
- The relationship between the optical Halpha filaments and the X-ray emission in the core of the Perseus cluster
- The cluster-scale AGN outburst in Hydra A
- Cold molecular gas in the Perseus cluster core - Association with X-ray cavity, Halpha filaments and cooling flow -
- Stirring Up the Pot: Can Cooling Flows In Galaxy Clusters Be Quenched By Gas Sloshing?
- X-ray Supercavities in the Hydra A Cluster and the Outburst History of the Central Galaxy's Active Nucleus
- Shocks and Cavities from Multiple Outbursts in the Galaxy Group NGC 5813: A Window to AGN Feedback
- Sloshing of the Magnetized Cool Gas in the Cores of Galaxy Clusters
- Atmospheric gas dynamics in the Perseus cluster observed with Hitomi
- Gas sloshing, cold front formation, and metal redistribution: the Virgo cluster as a quantitative test case
- A Very Deep Chandra Observation of the Galaxy Group NGC 5813: AGN Shocks, Feedback, and Outburst History
- A Very Deep Chandra Observation of Abell 2052: Bubbles, Shocks, and Sloshing
- Buoyant radio plasma in clusters of galaxies
- Cold fronts in galaxy clusters
- Simulating the interaction of jets with the intra-cluster medium
- MHD Simulations of AGN Jets in a Dynamic Galaxy Cluster Medium
- Gas sloshing, cold fronts, Kelvin-Helmholtz instabilities and the merger history of the cluster of galaxies Abell 496
- Constraining the Nature of X-ray Cavities in Clusters and Galaxies
- Precessing jets and X-ray bubbles from NGC1275 (3C84) in the Perseus galaxy cluster: a view from 3D numerical simulations
- Deep Chandra Observations of the Extended Gas Sloshing Spiral in A2029
- Cold Fronts: Probes of Plasma Astrophysics in Galaxy Clusters
- Precession of the Super-Massive Black Hole in NGC 1275 (3C 84)?
- Is there a giant Kelvin-Helmholtz instability in the sloshing cold front of the Perseus cluster?
- A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics
- Measuring bulk flows of the intracluster medium in the Perseus and Coma galaxy clusters using XMM-Newton
- Feedback through multiple outbursts in the cluster 2A 0335+096
- High-resolution VLA low radio frequency observations of the Perseus cluster: radio lobes, mini-halo and bent-jet radio galaxies
- LOFAR Observations of X-ray Cavity Systems
- What Do the Hitomi Observations Tell Us About the Turbulent Velocities in the Perseus Cluster? Probing the Velocity Field with Mock Observations
- How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relics
- On the Rayleigh-Taylor Instability of Radio Bubbles in Galaxy Clusters
- Inflating Fat Bubbles in Clusters of Galaxies by Precessing Massive Slow Jets
- Measuring sloshing, merging and feedback velocities in the Virgo cluster
- Simulating Astro-H Observations of Sloshing Gas Motions in the Cores of Galaxy Clusters
- Bubbles in Planetary Nebulae and Clusters of Galaxies: Jet Bending
- A detailed kinematic study of 3C 84 and its connection to Gamma-rays
- A new feedback cycle in the archetypal cooling flow group NGC 5044
- Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter