Cold gas in cluster cores: Global stability analysis and non-linear simulations of thermal instability
arXiv:1512.01217 · doi:10.1093/mnras/stw152
Abstract
We perform global linear stability analysis and idealized numerical simulations in global thermal balance to understand the condensation of cold gas from hot/virial atmospheres (coronae), in particular the intracluster medium (ICM). We pay particular attention to geometry (e.g., spherical versus plane-parallel) and the nature of the gravitational potential. Global linear analysis gives a similar value for the fastest growing thermal instability modes in spherical and Cartesian geometries. Simulations and observations suggest that cooling in halos critically depends on the ratio of the cooling time to the free-fall time (). Extended cold gas condenses out of the ICM only if this ratio is smaller than a threshold value close to 10. Previous works highlighted the difference between the nature of cold gas condensation in spherical and plane-parallel atmospheres; namely, cold gas condensation appeared easier in spherical atmospheres. This apparent difference due to geometry arises because the previous plane-parallel simulations focussed on {\em in situ} condensation of multiphase gas but spherical simulations studied condensation {\em anywhere} in the box. Unlike previous claims, our nonlinear simulations show that there are only minor differences in cold gas condensation, either in situ or anywhere, for different geometries. The amount of cold gas condensing depends on the shape of the gravitational potential well; gas has more time to condense if gravitational acceleration decreases toward the center. In our idealized simulations with heating balancing cooling in each layer, there can be significant mass/energy/momentum transfer across layers that can trigger condensation and drive far beyond the critical value close to 10. Triggered condensation is very prominent in plane-parallel simulations, in which a large amount of cold gas condenses out.
arXiv comment17 pages, 16 figures, 2 tables, version accepted in MNRAS. Links to python codes for global stability analysis: https://drive.google.com/folderview?id=0B2HaDXI2USsZWUdESVVsN2RGeVU&usp=sharing
References in corpus (27)
- The Structure of Cold Dark Matter Halos
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- The broken hierarchy of galaxy formation
- Heating Hot Atmospheres with Active Galactic Nuclei
- Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
- Thermal Instability in Gravitationally-Stratified Plasmas: Implications for Multi-Phase Structure in Clusters and Galaxy Halos
- Thermal Instability & the Feedback Regulation of Hot Halos in Clusters, Groups, and Galaxies
- Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets
- Simulating Radiating and Magnetized Flows in Multi-Dimensions with ZEUS-MP
- The Regulation of Cooling and Star Formation in Luminous Galaxies by AGN Feedback and the Cooling-Time/Entropy Threshold for the Onset of Star Formation
- Regulation of star formation in giant galaxies by precipitation, feedback, and conduction
- On the Nature of Feedback Heating in Cooling Flow Clusters
- On the Origin of the Extended Halpha Filaments in Cooling Flow Clusters
- Cooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters
- Modeling AGN Feedback in Cool-Core Clusters: The Formation of Cold Clumps
- Cool core cycles: Cold gas and AGN jet feedback in cluster cores
- Thermal Instability with Anisotropic Thermal Conduction and Adiabatic Cosmic Rays: Implications for Cold Filaments in Galaxy Clusters
- Anisotropic Thermal Conduction and the Cooling Flow Problem in Galaxy Clusters
- Gas Condensation in the Galactic Halo
- Thermal Instability in Clusters of Galaxies with Conduction
- On the Structure of Hot Gas in Halos: Implications for the Lx-Tx Relation & Missing Baryons
- Turbulence and cooling in galaxy cluster cores
- Growth and Evolution of Thermal Instabilities in Idealized Galaxy-Cluster Cores
- Thermal Conduction and Multiphase Gas in Cluster Cores
- Radiatively Inefficient Accretion Flow Simulations with Cooling: Implications for Black Hole Transients
- The cold mode: A phenomenological model for the evolution of density perturbations in the intracluster medium
- The HBI in a quasi-global model of the intracluster medium
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- A Global Model For Circumgalactic and Cluster-Core Precipitation
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- Hot Atmospheres, Cold Gas, AGN Feedback and the Evolution of Early Type Galaxies: a Topical Perspective
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- The Onset of Thermally Unstable Cooling from the Hot Atmospheres of Giant Galaxies in Clusters - Constraints on Feedback Models
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- Turbulence in the intracluster medium: simulations, observables & thermodynamics
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- Thermal Instability in the CGM of Galaxies: Testing "Precipitation" Models with the FIRE Simulations
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- The effect of rotation on the thermal instability of stratified galactic atmospheres - I. Local analysis
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- Constraints on precipitation-limited hot halos from massive galaxies to galaxy clusters
- Multiphase condensation in cluster halos: interplay of cooling, buoyancy and mixing
- AGN feedback with the Square Kilometer Array (SKA) and implications for cluster physics and cosmology
- Dynamical and thermal properties of the parsec-scale gases spherically accreted onto low luminous active galactic nuclei
- On the requirement for mixing-heating to utilize bubble cosmic rays to heat the intracluster medium
- CRexit: how different cosmic ray transport modes affect thermal instability in the circumgalactic medium
- Multiphase gas in elliptical galaxies: the role of Type Ia supernovae
- Deprojection of X-ray data in galaxy clusters: confronting simulations with observations
- Cold fronts in galaxy clusters I: A case for the large-scale global eigen modes in unmagnetized and weakly magnetized cluster core
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- Thermal instability through the outer half of quasi-static spherically symmetric molecular clumps and cores
- Acoustic waves and g-mode turbulence as energy carriers in a viscous intracluster medium