Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies

Abstract

Galaxy groups are more than an intermediate scale between clusters and halos hosting individual galaxies, they are crucial laboratories capable of testing a range of astrophysics from how galaxies form and evolve to large scale structure (LSS) statistics for cosmology. Cosmological hydrodynamic simulations of groups on various scales offer an unparalleled testing ground for astrophysical theories. Widely used cosmological simulations with ~(100 Mpc)^3 volumes contain statistical samples of groups that provide important tests of galaxy evolution influenced by environmental processes. Larger volumes capable of reproducing LSS while following the redistribution of baryons by cooling and feedback are essential tools necessary to constrain cosmological parameters. Higher resolution simulations can currently model satellite interactions, the processing of cool (T~10^4 K) multi-phase gas, and non-thermal physics including turbulence, magnetic fields, and cosmic ray transport. We review simulation results regarding the gas and stellar contents of groups, cooling flows and the relation to the central galaxy, the formation and processing of multi-phase gas, satellite interactions with the intragroup medium, and the impact of groups for cosmological parameter estimation. Cosmological simulations provide evolutionarily consistent predictions of these observationally difficult-to-define objects, and have untapped potential to accurately model their gaseous, stellar, and dark matter distributions.

arXiv comment61 pages, 18 figures, and 2 tables. This review article is part of the special issue "The Physical Properties of the Groups of Galaxies", edited by L. Lovisari and S. Ettori. Published in MDPI - Universe: https://www.mdpi.com/journal/universe/special_issues/PPGG

References in corpus (379)

• A Universal Density Profile from Hierarchical Clustering
• Galactic Stellar and Substellar Initial Mass Function
• On the variation of the Initial Mass Function
• Star Formation in Galaxies Along the Hubble Sequence
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Star Formation in the Milky Way and Nearby Galaxies
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Modeling feedback from stars and black holes in galaxy mergers
• Simulating Galaxy Formation with the IllustrisTNG Model
• First results from the IllustrisTNG simulations: matter and galaxy clustering
• First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
• Mass function of dark matter halos
• The hierarchical formation of the brightest cluster galaxies
• First results from the IllustrisTNG simulations: the galaxy color bimodality
• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
• Galactic star formation and accretion histories from matching galaxies to dark matter haloes
• Physical Models of Galaxy Formation in a Cosmological Framework
• First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• Radiative transfer in a clumpy universe: IV. New synthesis models of the cosmic UV/X-ray background
• GIZMO: A New Class of Accurate, Mesh-Free Hydrodynamic Simulation Methods
• Revising the Halofit Model for the Nonlinear Matter Power Spectrum
• FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation
• Simba: Cosmological Simulations with Black Hole Growth and Feedback
• The Circumgalactic Medium
• First results from the IllustrisTNG simulations: radio haloes and magnetic fields
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• On the Maximum Luminosity of Galaxies and Their Central Black Holes: Feedback From Momentum-Driven Winds
• First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
• The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment
• A model for cosmological simulations of galaxy formation physics
• The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation
• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time
• The Star-formation Mass Sequence out to z=2.5
• A unified model for AGN feedback in cosmological simulations of structure formation
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
• The physics driving the cosmic star formation history
• Reconstructing the linear power spectrum of cosmological mass fluctuations
• Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations--I. Isolated Galaxies
• Smoothed Particle Hydrodynamics and Magnetohydrodynamics
• Properties of Galaxy Groups in the SDSS: I.-- The Dependence of Colour, Star Formation, and Morphology on Halo Mass
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS)
• On the relation between the Schmidt and Kennicutt-Schmidt star formation laws and its implications for numerical simulations
• Gusty, gaseous flows of FIRE: galactic winds in cosmological simulations with explicit stellar feedback
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• Chandra imaging of the complex X-ray core of the Perseus cluster
• The Role of Pressure in GMC Formation II: The H_2 - Pressure Relation
• A deep Chandra observation of the Perseus cluster: shocks and ripples
• Galaxy evolution in groups and clusters: satellite star formation histories and quenching timescales in a hierarchical Universe
• Galaxy Zoo: the dependence of morphology and colour on environment
• Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
• Direct cosmological simulations of the growth of black holes and galaxies
• High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies
• Simulating galactic outflows with thermal supernova feedback
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• xCOLD GASS: the complete IRAM-30m legacy survey of molecular gas for galaxy evolution studies
• X-ray Spectroscopy of Cooling Clusters
• On the evolution of the HI column density distribution in cosmological simulations
• The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
• How Do Massive Black Holes Get Their Gas?
• Galaxy evolution in groups and clusters: star formation rates, red sequence fractions, and the persistent bimodality
• K-band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
• The Horizon-AGN simulation: morphological diversity of galaxies promoted by AGN feedback
• Feedback and Recycled Wind Accretion: Assembling the z=0 Galaxy Mass Function
• The Santa Barbara cluster comparison project: a comparison of cosmological hydrodynamics solutions
• The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
• An investigation of cooling flows and general cluster properties from an X-ray image deprojection analysis of 207 clusters of galaxies
• The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology
• The Aquila comparison Project: The Effects of Feedback and Numerical Methods on Simulations of Galaxy Formation
• The 2013 Release of Cloudy
• Cosmological simulations of black hole growth: AGN luminosities and downsizing
• 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
• Chaotic cold accretion onto black holes
• The Enrichment of the Intergalactic Medium with Adiabatic Feedback I: Metal Cooling and Metal Diffusion
• eROSITA Science Book: Mapping the Structure of the Energetic Universe
• The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses
• A Census of Baryons in Galaxy Clusters and Groups
• Smoothed Particle Hydrodynamics in Astrophysics
• Towards a realistic population of simulated galaxy groups and clusters
• Baryon effects on the internal structure of LCDM halos in the EAGLE simulations
• X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation
• The COS-Halos Survey: Rationale, Design, and A Census of Circumgalactic Neutral Hydrogen
• Chemical enrichment of galaxy clusters from hydrodynamical simulations
• Time-Dependent Ionization in Radiatively Cooling Gas
• Self-regulated growth of supermassive black holes by a dual jet/heating AGN feedback mechanism: methods, tests and implications for cosmological simulations
• 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
• Virgo Galaxies with Long One-Sided HI Tails
• Grackle: a Chemistry and Cooling Library for Astrophysics
• Evolution of the Galaxy - Dark Matter Connection and the Assembly of Galaxies in Dark Matter Halos
• How special are Brightest Group and Cluster Galaxies?
• MUFASA: Galaxy Formation Simulations With Meshless Hydrodynamics
• The Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs
• Galaxy Groups in the SDSS DR4: II. halo occupation statistics
• Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets
• A physical model for cosmological simulations of galaxy formation: multi-epoch validation
• Simulations of magnetic fields in isolated disk galaxies
• Stellar and total baryon mass fractions in groups and clusters since redshift 1
• Quantifying the effect of baryon physics on weak lensing tomography
• Locating the "missing" baryons with extragalactic dispersion measure estimates
• Galaxy Cluster Baryon Fractions Revisited
• The baseline intracluster entropy profile from gravitational structure formation
• A High Resolution Study of the Hydra A Cluster with Chandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling Flow
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• Systematics in the X-ray Cluster Mass Estimators
• The Origin of the Brightest Cluster Galaxies
• The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end
• The Birmingham-CfA cluster scaling project - III: entropy and similarity in galaxy systems
• The case for AGN feedback in galaxy groups
• Dark Matter Substructure in Numerical Simulations: A Tale of Discreteness Noise, Runaway Instabilities, and Artificial Disruption
• The impact of angular momentum on black hole accretion rates in simulations of galaxy formation
• The intragroup medium in loose groups of galaxies
• Feedback Heating by Cosmic Rays in Clusters of Galaxies
• The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
• An Analytic Model of Angular Momentum Transport by Gravitational Torques: From Galaxies to Massive Black Holes
• Pre-Processing of Galaxies before Entering a Cluster
• The Importance of Mergers for the Origin of Intracluster Stars in Cosmological Simulations of Galaxy Clusters
• Scaling Properties of a Complete X-ray Selected Galaxy Group Sample
• Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces
• Why does the environmental influence on group and cluster galaxies extend beyond the virial radius?
• Gravitational torque-driven black hole growth and feedback in cosmological simulations
• Galaxies-Intergalactic Medium Interaction Calculation --I. Galaxy formation as a function of large-scale environment
• The Minimum Universal Metal Density Between Redshifts of 1.5 and 5.5
• Cold gas stripping in satellite galaxies: from pairs to clusters
• Draping of Cluster Magnetic Fields over Bullets and Bubbles -- Morphology and Dynamic Effects
• Gas Stripping in Simulated Galaxies with a Multiphase ISM
• Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology
• Joint Analysis of Cluster Observations: II. Chandra/XMM-Newton X-ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies
• Regulation of star formation in giant galaxies by precipitation, feedback, and conduction
• The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
• Galactic winds driven by cosmic-ray streaming
• Probing Galactic Halos with Fast Radio Bursts
• The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications
• The Hydrangea simulations: galaxy formation in and around massive clusters
• The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme
• Gas expulsion by quasar-driven winds as a solution to the over-cooling problem in galaxy groups and clusters
• Raining on black holes and massive galaxies: the top-down multiphase condensation model
• The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
• Cool Core Clusters from Cosmological Simulations
• SZ effects in the Magneticum Pathfinder Simulation: Comparison with the Planck, SPT, and ACT results
• A new method to quantify the effects of baryons on the matter power spectrum
• Simulations of AGN feedback in galaxy clusters and groups: impact on gas fractions and the Lx-T scaling relation
• Bimodality of low-redshift circumgalactic O VI in non-equilibrium EAGLE zoom simulations
• Modified-Entropy Models for the Intracluster Medium
• The Impact of Enhanced Halo Resolution on the Simulated Circumgalactic Medium
• Cooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters
• AGN Feedback and Cooling Flows: Problems with Simple Hydrodynamical Models
• Regulation of the X-ray luminosity of clusters of galaxies by cooling and supernova feedback
• A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations
• The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
• Resolving small-scale cold circumgalactic gas in TNG50
• The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
• The impact of baryons on the matter power spectrum from the Horizon-AGN cosmological hydrodynamical simulation
• Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
• The stellar-to-halo mass relation over the past 12 Gyr
• Pre-Heated Isentropic Gas in Groups of Galaxies
• Calibrating the Nonlinear Matter Power Spectrum: Requirements for Future Weak Lensing Surveys
• Cosmic ray transport in galaxy clusters: implications for radio halos, gamma-ray signatures, and cool core heating
• Off the Beaten Path: A New Approach to Realistically Model The Orbital Decay of Supermassive Black Holes in Galaxy Formation Simulations
• Global simulations of galactic winds including cosmic ray streaming
• An MHD Gadget for cosmological simulations
• The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
• Physical Implications of the X-ray Properties of Galaxy Groups and Clusters
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
• Characterizing Circumgalactic Gas around Massive Ellipticals at z~0.4 - II. Physical Properties and Elemental Abundances
• Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
• The Evolution of Substructure in Galaxy, Group and Cluster Haloes I: Basic Dynamics
• Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• Properties of the Circumgalactic Medium in Cosmic Ray-Dominated Galaxy Halos
• X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: Tracing the evolution of AGN feedback in clusters of galaxies out to z=1.2
• The Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos
• Cosmic ray feedback in the FIRE simulations: constraining cosmic ray propagation with GeV gamma ray emission
• Explaining the entropy excess in clusters and groups of galaxies without additional heating
• Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
• Linking Macro, Meso, and Micro Scales in Multiphase AGN Feeding and Feedback
• The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field
• Dark matter haloes determine the masses of supermassive black holes
• Ram pressure feeding super-massive black holes
• On the role of AGN feedback on the thermal and chemodynamical properties of the hot intra-cluster medium
• Cooler and smoother -- the impact of cosmic rays on the phase structure of galactic outflows
• Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations
• Star formation quenching in simulated group and cluster galaxies: When, how, and why?
• Cool core cycles: Cold gas and AGN jet feedback in cluster cores
• Resurrecting the Red from the Dead: Optical Properties of BCGs in X-ray Luminous Clusters
• Jellyfish galaxies with the IllustrisTNG simulations: I. Gas-stripping phenomena in the full cosmological context
• Non-Equilibirum ionisation and cooling of metal-enriched gas in the presence of a photo-ionisation background
• The FABLE simulations: A feedback model for galaxies, groups and clusters
• SPHGal: Smoothed Particle Hydrodynamics with improved accuracy for Galaxy simulations
• Modeling AGN Feedback in Cool-Core Clusters: The Balance between Heating and Cooling
• The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes
• The fraction of cool-core clusters in X-ray vs. SZ samples using Chandra observations
• Thermal Instability with Anisotropic Thermal Conduction and Adiabatic Cosmic Rays: Implications for Cold Filaments in Galaxy Clusters
• Feedback from Active Galactic Nuclei in Galaxy Groups
• The Atacama Cosmology Telescope: Modeling the Gas Thermodynamics in BOSS CMASS galaxies from Kinematic and Thermal Sunyaev-Zel'dovich Measurements
• Testing the Low-Mass End of X-Ray Scaling Relations with a Sample of Chandra Galaxy Groups
• On the Origin of Cores in Simulated Galaxy Clusters
• The Role of Cosmic Ray Transport in Shaping the Simulated Circumgalactic Medium
• Introducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution
• Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations
• Are Radio AGN Powered by Accretion or Black Hole Spin?
• The Effects of Gas Dynamics, Cooling, Star Formation, and Numerical Resolution in Simulations of Cluster Formation
• A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• The Evolution of Central Group Galaxies in Hydrodynamical Simulations
• Cosmic Ray Streaming in Clusters of Galaxies
• Investigating the velocity structure and X-ray observable properties of simulated galaxy clusters with PHOX
• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• Towards a Holistic View of the Heating and Cooling of the Intracluster Medium
• Cosmic ray-driven galactic winds: streaming or diffusion?
• SIXTE -- The Generic X-ray Instrument Simulation Toolkit
• Anisotropic Diffusion in Mesh-Free Numerical Magnetohydrodynamics
• An observer's view of simulated galaxies: disc-to-total ratios, bars, and (pseudo-)bulges
• Cosmic-ray hydrodynamics: Alfvén-wave regulated transport of cosmic rays
• Models of the ICM with Heating and Cooling: Explaining the Global and Structural X-ray Properties of Clusters
• 3D simulations of viscous dissipation in the intracluster medium
• Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
• The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
• Cosmic distribution of highly ionized metals and their physical conditions in the EAGLE simulations
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
• High Redshift Metals I.: The Decline of C IV at z > 5.3
• A New Numerical Scheme for Cosmic Ray Transport
• Overconsumption, outflows and the quenching of satellite galaxies
• The X-ray Halo Scaling Relations of Supermassive Black Holes
• Metals in the IGM approaching the re-ionization epoch: results from X-shooter at the VLT
• A census of cool core galaxy clusters in IllustrisTNG
• The environmental dependence of HI in galaxies in the EAGLE simulations
• Ion-by-ion Cooling efficiencies
• Tracing the Reionization-Epoch Intergalactic Medium with Metal Absorption Lines
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• Where Are the Baryons? III: Non-Equilibrium Effects and Observables
• Role of Cosmic Rays in the Circumgalactic Medium
• Galaxy And Mass Assembly (GAMA): the Stellar Mass Budget by Galaxy Type
• Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies
• X-Ray Scaling Relations of Galaxy Groups in a Hydrodynamic Cosmological Simulation
• The Impact of Cosmic Rays on Thermal Instability in the Circumgalactic Medium
• Diffuse Baryons in Groups and Clusters of Galaxies
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - II: Size-luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass
• Quenching of Satellite Galaxies at the Outskirts of Galaxy Clusters
• Scaling Properties of Galaxy Groups
• The Complete Local Volume Groups Sample - I. Sample Selection and X-ray Properties of the High-Richness Subsample
• The three phases of galaxy formation
• Cycling of the powerful AGN in MS 0735.6+7421 and the duty cycle of radio AGN in Clusters
• Star Formation Feedback and Metal Enrichment History Of The Intergalactic Medium
• The dependence of cosmic ray driven galactic winds on halo mass
• Line Overlap and Self-Shielding of Molecular Hydrogen in Galaxies
• nIFTy galaxy cluster simulations I: dark matter & non-radiative models
• AGN heating and dissipative processes in galaxy clusters
• A hydrodynamical halo model for weak-lensing cross correlations
• Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
• Testing Sunyaev-Zel'dovich measurements of the hot gas content of dark matter haloes using synthetic skies
• Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
• Can AGN feedback break the self-similarity of galaxies, groups, and clusters?
• The Effect of Environment on the Formation of Halpha Filaments and Cool Cores in Galaxy Groups and Clusters
• Physical viscosity in smoothed particle hydrodynamics simulations of galaxy clusters
• Heating of the intracluster medium by quasar outflows
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• The environmental dependence of gas accretion onto galaxies: quenching satellites through starvation
• Southern GEMS Groups I: Dynamical Properties
• Which AGN Jets Quench Star Formation in Massive Galaxies?
• Star Formation Efficiency in the Cool Cores of Galaxy Clusters
• The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
• Detection of Diffuse Neutral Intragroup Medium in Hickson Compact Groups
• Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
• On the impact of baryons on the halo mass function, bias, and cluster cosmology
• Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
• The Last Eight-Billion Years of Intergalactic CIV Evolution
• Enrichment and Pre-Heating in Intragroup Gas from Galactic Outflows
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• The Hot Gas Halos of Galaxies in Groups
• The separate and combined effects of baryon physics and neutrino free-streaming on large-scale structure
• A Survey of MgII Absorption at 2 < z < 6 with Magellan / FIRE: I: Sample and Evolution of the MgII Frequency
• General Requirements on Matter Power Spectrum Predictions for Cosmology with Weak Lensing Tomography
• The fate of disk galaxies in IllustrisTNG clusters
• An EAGLE's View of Ex-situ Galaxy Growth
• The Hubble Sequence in Groups: The Birth of the Early-Type Galaxies
• Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN
• Effects of Different Cosmic Ray Transport Models on Galaxy Formation
• The luminosity -- halo-mass relation for brightest cluster galaxies
• On The Efficiency of Jet Production in Radio Galaxies
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters
• Evidence for recent star formation in BCGs: a correspondence between blue cores and UV excess
• Triggering and Delivery Algorithms for AGN Feedback
• The high molecular gas content, and the efficient conversion of neutral into molecular gas, in jellyfish galaxies
• Cosmic ray heating in cool core clusters - II. Self-regulation cycle and non-thermal emission
• The Gas-Phase Metallicity of Central and Satellite Galaxies in the SDSS
• BCG Mass Evolution in Cosmological Hydro-Simulations
• MAGIICAT VI. The MgII Intragroup Medium is Kinematically Complex
• AGN contamination of galaxy-cluster thermal X-ray emission: predictions for eRosita from cosmological simulations
• Observing simulated galaxy clusters with PHOX: a novel X-ray photon simulator
• Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• Dependency of halo concentration on mass, redshift and fossilness in Magneticum hydrodynamic simulations
• The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations
• A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
• The contributions of matter inside and outside of haloes to the matter power spectrum
• Correlation Between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies
• Cool-Core Clusters : Role of BCG, Star Formation & AGN-Driven Turbulence
• Feedback from Reorienting AGN Jets
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• Star formation rates and stellar masses from machine learning
• The pressure profiles of hot gas in local galaxy groups
• On the origin of gas-poor galaxies in galaxy clusters using cosmological hydrodynamic simulations
• EAGLE and Illustris-TNG predictions for resolved eROSITA X-ray observations of the circumgalactic medium around normal galaxies
• A Chandra study of the large-scale shock and cool filaments in Hydra A: Evidence for substantial gas dredge-up by the central outburst
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• AGN jet-driven stochastic cold accretion in cluster cores
• The Soft, Fluctuating UVB at $z\sim 6$ as Traced by C IV, SiIV, and CII
• The EAGLE simulations of galaxy formation: Public release of particle data
• The competition between confinement and ram pressure and its implications for galaxies in groups and clusters
• Warm-hot Gas in X-ray Bright Galaxy Clusters and the H I-deficient Circumgalactic Medium in Dense Environments
• The better half -- Asymmetric star-formation due to ram pressure in the EAGLE simulations
• Isotropic Heating of Galaxy Cluster Cores via Rapidly Reorienting AGN Jets
• A Link Between Ram Pressure Stripping and Active Galactic Nuclei
• The origin of the enhanced metallicity of satellite galaxies
• The Multi-Epoch Nearby Cluster Survey: type Ia supernova rate measurement in z~0.1 clusters and the late-time delay time distribution
• How To Light It Up: Simulating Ram-Pressure Stripped X-ray Bright Tails
• Enrichment of the hot intracluster medium: numerical simulations
• Warm Gas in the Virgo Cluster: I. Distribution of Lya Absorbers
• The Growth and Enrichment of the Intragroup Gas
• Characterizing hydrostatic mass bias with Mock-X
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• The regulation of star formation in cool-core clusters: imprints on the stellar populations of brightest cluster galaxies
• GASP XXXIV: Unfolding the thermal side of ram pressure stripping in the jellyfish galaxy JO201
• How baryons can significantly bias cluster count cosmology
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• Fountains and storms: The role of AGN and mergers in disrupting the cool-core in the RomulusC simulation
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• Diversity in the stellar velocity dispersion profiles of a large sample of Brightest Cluster Galaxies $z\le 0.3$
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• The Temperature Structure of the Warm-Hot Intergalactic Medium
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• The Impact of the Group Environment on the OVI Circumgalactic Medium
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Constraining star formation rates in cool-core brightest cluster galaxies
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
• Galaxy And Mass Assembly: search for a population of high-entropy galaxy groups
• Thermal Instability in the CGM of $L_{\star }$ Galaxies: Testing "Precipitation" Models with the FIRE Simulations
• Morphology and kinematics of orbital components in CALIFA galaxies across the Hubble sequence
• Mixing matters
• The Relationship Between Brightest Cluster Galaxy Star Formation and the Intracluster Medium in CLASH
• Extending the $L_{\mathrm{X}}-T$ relation from clusters to groups-Impact of cool core nature, AGN feedback, and selection effects
• The UV-upturn in brightest cluster galaxies
• Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy Survey
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• Lyman-alpha Absorbers and the Coma Cluster
• Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
• Brightest Group Galaxies: Stellar Mass and Star Formation Rate (paper I)
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
• Simulating the Carbon Footprint of Galactic Halos
• The trajectories of galaxies in groups: mass loss and preprocessing
• The Ultraviolet Detection of Diffuse Gas in Galaxy Groups
• Density Profiles of Collisionless Equilibria. II. Anisotropic Spherical Systems
• Discovery of an HI-rich Gas Reservoir in the Outskirts of SZ-effect Selected Clusters
• Powering of H$\alpha$ filaments by cosmic rays
• C IV absorbers tracing cool gas in dense galaxy group/cluster environments
• The challenging task of determining star formation rates: the case of a massive stellar burst in the brightest cluster galaxy of Phoenix galaxy cluster
• The special growth history of central galaxies in groups and clusters
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• COS Observations of the Cosmic Web: A Search for the Cooler Components of a Hot, X-ray Identified Filament
• Detection of Metal-Rich, Cool-Warm Gas in the Outskirts of Galaxy Clusters
• Toward the low-scatter selection of X-ray clusters: Galaxy cluster detection with eROSITA through cluster outskirts
• Stellar Mass and 3.4 $\mu$m M/L Ratio Evolution of Brightest Cluster Galaxies in COSMOS since z ~ 1.0
• The BACCO Simulation Project: A baryonification emulator with Neural Networks

Cited by in corpus (55)

• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• The importance of black hole repositioning for galaxy formation simulations
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• Gas condensation in Brightest Group Galaxies unveiled with MUSE
• Deep Synoptic Array science: Two fast radio burst sources in massive galaxy clusters
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• The MUSE Extremely Deep Field: a first panoramic view of an Mg II emitting intragroup medium
• Mapping "out-of-the-box" the properties of the baryons in massive halos
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• Merger histories of brightest group galaxies from MUSE stellar kinematics
• EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• The Three Hundred Project: the evolution of physical baryon profiles
• The Complete Local Volume Groups Sample -- IV. Star formation and gas content in group-dominant galaxies
• The Obsidian model: Three regimes of black hole feedback
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
• $i(cm)z$, a semi-analytic model for the thermodynamic properties in galaxy clusters: calibrations with mass and redshift, and implication for the hydrostatic bias
• Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters
• Constraints on Self-Interacting dark matter from relaxed galaxy groups
• COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• The perils of stacking optically selected groups in eROSITA data. The Magneticum perspective
• Simulated [CII] in high-z galaxies
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• Measuring cosmic filament spin with the kinetic Sunyaev-Zel'dovich effect
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• The Three Hundred Project: Modeling Baryon and Hot-Gas Fraction Evolution in Simulated Clusters
• Scaling relations of clusters and groups, and their evolution
• Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters
• Modelling the selection of galaxy groups with end to end simulations
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Energetic particles and high-energy processes in cosmological filaments and their astronomical implications
• Strong Evidence for Cosmic Ray-Supported $\sim$L${}^{\ast }$ Galaxy Halos via X-ray \& tSZ Constraints
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
• Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• MUSE-ALMA Haloes XIII. Molecular gas in $z\sim 0.5$ HI-selected galaxies
• Modelling gas around galaxy pairs and groups using the Q0107 quasar triplet
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• The Cen A galaxy group: dynamical mass and missing baryons
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Bound or blown: the fate of hot gas in galaxy groups
• Studying the gaseous outskirts of galaxy groups with coherent Ly alpha absorption patterns