Simulations of X-ray Clusters

Abstract

We present simulations of the formation and evolution of galaxy clusters in the Cold Dark Matter cosmogony. Clusters with a wide range of mass were selected from previous N-body models, and were resimulated at higher resolution using a combined N-body/Smooth Particle Hydrodynamics code. The effects of radiative cooling on the gas are neglected. While many present-day clusters are predicted to be undergoing mergers, the density profiles of those that are approximately in equilibrium are all very similar, both for the gas and for the dark matter. These profiles show no sign of a uniform density core and steepen gradually from the centre outwards. The standard $\beta$-model is a reasonable fit over most of the radius range observable in real clusters. However, the value obtained for the slope parameter ${\beta }_f$ increases with the outermost radius of the fit. Temperature profiles of different simulated clusters are also similar. Typically the temperature is almost uniform in the regions which emit most of the X-ray flux but drops at larger radii. The gas temperature and dark matter velocity dispersion in equilibrium clusters give values of ${\beta }_T\equiv \mu m_p{\sigma }_{DM}^2/kT$ which are consistent with unity provided an X-ray emission-weighted temperature is used. Larger values of ${\beta }_T$ are found in merging objects where there is a transient boost in the velocity dispersion of the system. Thus ${\beta }_T>1$ may be an observational indicator of merging in real clusters. The similar structure of clusters of differing mass results in scaling relations between the X-ray and dynamical properties of clusters identified at

uuencoded file, 14 pages, figures from dust0.dur.ac.uk (129.234.8.70), /pub/jfn/xrclus_fig_ps.tar.Z

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• Gamma-ray and synchrotron emission from neutralino annihilation in the Large Magellanic Cloud
• The effect of tides on the Fornax dwarf spheroidal galaxy
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• Observation of small scale structure using sextupole lensing
• Galaxy cluster number count data constraints on cosmological parameters
• Entropy profiles in X-ray luminous galaxy clusters at z>0.1
• Entropy of gas and dark matter in galaxy clusters
• Merger traces in the spatial distribution of stellar populations in the Fornax dSph galaxy
• MAGI: many-component galaxy initialiser
• Constraints from the Hubble Deep Field on High Redshift Quasar Models
• High-Resolution Optical Rotation Curves of Low-Luminosity Spiral Galaxies
• The luminosity functions and stellar masses of galactic disks and spheroids
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• Weak lensing analysis of MS 1008-1224 with the VLT
• Are Clusters Standard Candles? Galaxy Cluster Scaling Relations With the Sunyaev-Zeldovich Effect
• Probing Cosmology with the X-ray Forest
• The formation of galaxy disks in a hierarchical universe
• Multiwavelength evidence of the physical processes in radio jets
• Merging Cold Fronts in the Galaxy Pair NGC 7619 and NGC 7626
• Detecting Sunyaev-Zel'dovich clusters with PLANCK: I. Construction of all-sky thermal and kinetic SZ-maps
• Adiabatic scaling relations of galaxy clusters
• Axion Miniclusters Made Easy
• Galaxy cluster mergers
• Chandra and XMM-Newton Observations of NGC 4214: The Hot Interstellar Medium and the Luminosity Function of Dwarf Starbursts
• Galaxy Models with Tangentially Anisotropic Velocity Distributions
• The effects of baryonic cooling on the concentration-mass relation
• Towards a characterization of X-ray galaxy clusters for cosmology
• Detection of Bulk Motions in the ICM of the Centaurus Cluster
• Constraints on the dynamical evolution of the galaxy group M81
• New Light on the Baryon Fraction in Galaxy Clusters
• The Cold Dark Matter crisis on galactic and subgalactic scales
• Effects of Quasar Feedback in Galaxy Groups
• Statistics and implications of substructure detected in a representative sample of X-ray clusters
• Mirror Matter, Mirror Gravity and Galactic Rotational Curves
• The baryonic mass-velocity relation; clues to feedback processes during structure formation and the cosmic baryon inventory
• Using Weak Lensing to find Halo Masses
• Angular momentum transfer to a Milky Way disk at high redshift
• Cosmological Simulations of the Preheating Scenario for Galaxy Cluster Formation: Comparison to Analytic Models and Observations
• Bright and Dark Matter in Elliptical Galaxies: Mass and Velocity Distributions from Self-consistent Hydrodynamical Simulations
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• Radio Emission in the Cosmic Web
• First detection of a virial shock with SZ data: implication for the mass accretion rate of Abell 2319
• Nonthermal emission from clusters of galaxies
• Internal rotation of Milky Way dwarf spheroidal satellites with $Gaia$ Early Data Release 3
• The HI Velocity Function: a test of cosmology or baryon physics?
• Predicting the Clustering of X-Ray Selected Galaxy Clusters in Flux-Limited Surveys
• Modelling Shear Flows with SPH and Grid Based Methods
• The morphological and dynamical evolution of simulated galaxy clusters
• Compact groups in theory and practice -- IV. The connection to large-scale structure
• Temperature Map of the Perseus Cluster of Galaxies Observed with ASCA
• An Unbiased Measurement of Ho through Cosmic Background Imager Observations of the Sunyaev-Zel'dovich Effect in Nearby Galaxy Clusters
• Determinations of Key Physical Parameters Related to Classical Double Radio Sources
• Empirical Determinations of Key Physical Parameters Related to Classical Double Radio Sources
• X-ray Measurements of the Gravitational Potential Profile in the Central Region of the Abell 1060 Cluster of Galaxies
• Kinematics and Mass Profile of AWM 7
• Disc-like Objects in Hierarchical Hydrodynamical Simulations: Comparison with Observations
• The dark matter distribution in z~0.5 clusters of galaxies. I : Determining scaling relations with weak lensing masses
• Gravitational redshift profiles in the $f(R)$ and symmetron models
• The power spectrum amplitude from clusters revisited: σ_8 using simulations with preheating and cooling
• Tidally induced bars in dwarf galaxies on different orbits around a Milky Way-like host
• X-ray modelling of galaxy cluster gas and mass profiles
• Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-ray, SZ, and Lensing Data
• A cosmological context for compact massive galaxies
• Chandra Observations of low velocity dispersion groups
• Properties of the double beta model for intracluster gas
• Cool circumgalactic gas of passive galaxies from cosmological inflow
• 2dFGRS and SDSS Galaxy Group Density Profiles
• Star Formation and Feedback in Dwarf Galaxies
• Comparisons of Cluster Mass Determinations by X-ray Observations and Gravitational Lensing
• A dynamics-based density profile for dark haloes -- II. Fitting function
• A comparison of the strong lensing properties of the Sersic and the NFW profiles
• SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias
• An XMM-Newton observation of the galaxy group MKW 4
• Kiloparsec Mass/Light Offsets in the Galaxy Pair-Ly$\alpha$ Emitter Lens System SDSS\,J1011$+$0143
• Entropy principle and complementary second law of thermodynamics for self-gravitating systems
• The Influence of Concentration and Dynamical State on Scatter in the Galaxy Cluster Mass-Temperature Relation
• Global cluster morphology and its evolution: X-ray data vs CDM, LCDM and mixed models
• Theoretical Uncertainties due to AGN Subgrid Models in Predictions of Galaxy Cluster Observable Properties
• Suzaku Observation of HCG 62: Temperature, Abundance, and Extended Hard X-ray Emission Profiles
• On the contribution of microlensing to X-ray variability of high-redshifted QSOs
• Weak Gravitational Lensing by a Sample of X-Ray Luminous Clusters of Galaxies -- II. Comparison with Virial Masses
• The Scale-Invariant Vacuum (SIV) Theory: A Possible Origin of Dark Matter and Dark Energy
• The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VII The Mass Function of Galaxy Clusters
• Sunyaev-Zel'dovich profiles and scaling relations: modelling effects and observational biases
• Effects of Disks on Gravitational Lensing by Spiral Galaxies
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• A Chandra Study of Temperature Substructures in Intermediate-Redshift Galaxy Clusters
• On the origin of the Tully-Fisher relation
• GOTHIC: Gravitational oct-tree code accelerated by hierarchical time step controlling
• Constraining q_0 with Cluster Gas Mass Fractions: A Feasibility Study
• XMM observes ClJ0152.7-1357: A massive galaxy cluster forming at merger crossroads at z=0.83
• Effects of the halo concentration distribution on strong-lensing optical depth and X-ray emission
• The Lives of High Redshift Mergers
• Lensing Sunyaev-Zel'dovich Clusters
• Fast Identification of Bound Structures in Large N-body Simulations
• Clues on Regularity in the Structure and Kinematics of Elliptical Galaxies from Self-consistent Hydrodynamical Simulations: the Dynamical Fundamental Plane
• Stellar Population Trends in S0 Galaxies
• The orbital structure of a tidally induced bar
• Joint X-Ray and Optical Measurements of the Mass Distribution of the Distant Galaxy Cluster CLJ 0152.7-1357
• Cosmological simulations of Milky Way-sized galaxies
• The X-ray Fundamental Plane and $L_X-T$ Relation of Clusters of Galaxies
• Gravitational Lensing with Three-Dimensional Ray Tracing
• The 400d Galaxy Cluster Survey weak lensing programme: II: Weak lensing study of seven clusters with MMT/Megacam
• Colour Evolution of Disk Galaxy Models from z=4 to z=0
• Radio emission from dark matter annihilation in the Large Magellanic Cloud
• Numerical convergence of physical variables in hydrodynamical simulations of cooling clusters
• Self-similar collapse and the structure of dark matter halos: A fluid approach
• XMM-Newton observations of two X-ray bright galaxy groups - pushing out to r_500
• The impact of massive stars and black holes on the fate of open star clusters and their tidal streams
• Cosmology Using Cluster Internal Velocity Dispersions
• An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
• An XMM-Newton study of the RGH 80 galaxy group
• Metal distributions out to 0.5 r180 in the intracluster medium of four galaxy groups observed with Suzaku
• Cosmic rays through the Higgs portal
• The Dark Matter Haloes of Chandra X-ray Galaxy Clusters and Baryons Effect
• Chemical and Photometric Evolution of the Local Group Galaxy NGC 6822 in a Cosmological Context
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• Chandra X-Ray Spectroscopy and Imaging of the Galaxy Cluster PKS 0745-191
• X-ray Measurement of Dark Matter "Temperature" in Abell 1795
• X-ray temperature spectroscopy of simulated cooling clusters
• Peculiar acceleration
• Could pressureless dark matter have pressure?
• Building a cluster: shocks, cavities, and cooling filaments in the group-group merger NGC 6338
• Magnetic field amplification and X-ray emission in galaxy minor mergers
• Universal predictions of screened modified gravity on cluster scales
• X-ray and strong lensing mass estimate of MS2137.3-2353
• Building the Stellar Halo Through Feedback in Dwarf Galaxies
• Infrared observations of gravitational lensing in Abell 2219 with CIRSI
• On the tidal radius of satellites on prograde and retrograde orbits
• Baryon Distribution in Galaxy Clusters as a Result of Sedimentation of Helium Nuclei
• Photoionized Gas in Dark-Matter Minihalos in the Galactic Halo and Local Group
• Weak Lensing Mass Reconstruction of the Galaxy Cluster Abell 209
• The Expected Properties of Dark Lenses
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• The detection of diffuse emission in HCG 16 with XMM-Newton
• A 15-Kiloparsec X-Ray Disk in the Elliptical Galaxy NGC 1700
• Time-Delay Effect on the cOsmic Background Radiation by Static Gravitational Potential of Clusters
• Weak lensing measurements of the APEX-SZ galaxy cluster sample
• Smooth Particle Lensing
• The clustering of baryonic matter. I: a halo-model approach
• The serendipitous observation of a gravitationally lensed galaxy at z = 0.9057 from the Blanco Cosmology Survey: The Elliot Arc
• Studying the Dynamical Properties of 20 Nearby Galaxy Clusters
• A theorem on central velocity dispersions
• Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters
• Shape of the Galactic Orbits in Clusters
• Investigation of two colliding solitonic cores in Fuzzy Dark Matter models
• A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10${}^{15}$M${}_{\odot }$ Galaxy Cluster at z=0.7
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• A Baryonic Effect on the Merger Timescale of Galaxy Clusters
• The anatomy of the NGC 5044 group - I. Group membership and dynamics
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy
• H-Band and Spectroscopic Properties of Abell 1644
• X-ray and lensing results on the cluster around the powerful radio galaxy 4C+55.16
• A theoretical study of the luminosity temperature relation for clusters of galaxies
• Modified Virial Formulae and the Theory of Mass Estimators
• Tidally induced bars in gas-rich dwarf galaxies orbiting the Milky Way
• The Effect of Substructure on Mass Estimates of Galaxies
• Gamma-ray signatures of annihilation to charged leptons in dark matter substructure
• The truncation of stellar discs: the magnetic hypothesis
• Dark matter protohalos in MSSM-9 and implications for direct and indirect detection
• Cosmological black holes: the spherical perfect fluid collapse with pressure in a FRW background
• The Impact of Cluster Structure and Dynamical State on Scatter in the Sunyaev-Zel'dovich Flux-Mass Relation
• A Survey for Large Separation Lensed FIRST Quasars
• An accurate method of modeling cluster scaling relations in modified gravity
• The structure of Andromeda II dwarf spheroidal galaxy
• The Baryonic and Dark Matter Distributions in Abell 401
• Accretion of a satellite onto a spherical galaxy. II. Binary evolution and orbital decay
• Correlation Between the Halo Concentration (c) and the Virial Mass (Mvir) Determined from X-ray Clusters
• On the Probability Distribution of Cosmological Microlensing Optical Depths
• ROSAT X-ray Observations of the Cooling Flow Cluster A2597
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• Consequences of short range interactions between dark matter and protons in galaxy clusters
• Hot atmospheres of galaxies, groups, and clusters of galaxies
• Constraint on the mass of fuzzy dark matter from the rotation curve of the Milky Way
• Stellar-mass black holes in the Hyades star cluster?
• The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation histories
• Temperature and total mass profiles of the A3571 cluster of galaxies
• Morphology of low-redshift compact galaxy clusters I. Shapes and radial profiles
• Gas clump formation via thermal instability in high-redshift dwarf galaxy mergers
• The 21-cm signals from ultracompact minihalos as a probe of primordial small-scale fluctuations
• The Galaxy Cluster Luminosity-Temperature Relationship and Iron Abundances - A Measure of Formation History ?
• Determining cosmological parameters from X-ray measurements of strong lensing clusters
• Discriminating power of milli-lensing observations for dark matter models
• JWST's first glimpse of a z > 2 forming cluster reveals a top-heavy stellar mass function
• Mixed Models with n>1 and Large Scale Structure constraints
• Data-Based Optimal Bandwidth for Kernel Density Estimation of Statistical Samples
• The X-ray Luminosity Function of Nearby Rich and Poor Clusters of Galaxies: A Cosmological Probe
• On the radial density profile of intracluster gas tracing the isothermal dark halo with a finite core
• Simple Models for the Distribution of Dark Matter
• A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters
• Can Strong Gravitational Lensing Constrain Dark Energy?
• A physical and concise halo model based on the depletion radius
• A comprehensive analysis of NGC 2158 in Gaia era: photometric parameters, apex and orbit
• Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
• High-Resolution Simulations of Cluster Formation
• Galaxy-Galaxy Lensing by Non-Spherical Haloes I:Theoretical Considerations
• Stacking Clusters in the ROSAT All-Sky Survey
• Cluster Mass Estimate and a Cusp of the Mass Density Distribution in Clusters of Galaxies
• A Photometric and Kinematic Study of AWM 7
• Evidence for new physics from clusters ?
• The potential-energy tensors for subsystems. IV. Homeoidally striated density profiles with a central cusp
• The probability distribution of cluster formation times and implied Einstein Radii
• X-Ray observations of a subhalo associated with the NGC 4839 group infalling toward the Coma cluster
• Simulated evolution of the dark matter large-scale structure
• Gravitational lensing in low-redshift clusters of galaxies: the arc-like object in Abell 3408 and its lensing interpretation
• Implications of Halo Inside-out Growth on the X-Ray Properties of Nearby Galaxy Systems within the Preheating Scenario
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Gravitational Lensing by a structure in a cosmological background
• On the absence of gravitational lensing of the cosmic microwave background
• Sunyaev--Zel'dovich profile fitting with joint AMI-Planck analysis
• Gravitational redshifting of galaxies in the SPIDERS cluster catalogue
• Clusters of galaxies: setting the stage
• Satellite content and quenching of star formation in galaxy groups at z~1.8
• Mass estimation in the outer non-equilibrium region of galaxy clusters
• Where are the missing baryons in clusters?
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
• Impact of a non-Gaussian density field on Sunyaev-Zeldovich observables
• A universal angular momentum profile for dark matter haloes
• The local rotation curve of the Milky Way based on SEGUE and RAVE data
• The Celestial Buffet: multiple populations and globular cluster formation in dwarf galaxies
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
• Weak lensing density profiles and mass reconstructions of the galaxy clusters Abell 1351 and Abell 1995
• Radial orbit instability in dwarf dark matter haloes
• Synthetic X-ray and radio maps for two different models of Stephan's Quintet
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• The mass and dynamical state of Abell 2218
• Precision cosmology with baryons: non-radiative hydrodynamics of galaxy groups
• The mass and temperature functions in a moving barrier model
• Cluster abundance and large scale structure
• Probing the structure of the cold dark matter halo with ancient mica
• The Dark Matter Tidal Stripping History of the Sagittarius Core with N-body simulations
• AGN effect on cooling flow dynamics
• On the Detectability of the SZ Effect of Massive Young Galaxies
• Constraining the intracluster pressure profile from the thermal SZ power spectrum
• Abundance and evolution of galaxy clusters in cosmological models with massive neutrino
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Modelling the dynamical friction timescale of sinking satellite
• Systematic errors in the determination of Hubble constant due to the asphericity and non-isothermality of clusters of galaxies
• Spitzer observations of Abell 1763 - II: Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton data
• Empirical constraints on alternative gravity theories from gravitational lensing
• Galaxy rotation favors prolate dark matter haloes
• Lensing effects in inhomogeneous cosmological models
• CMB and Large Scale Structure as a test of Mixed Models with n>1
• Gas and Dark Matter Spherical Dynamics
• Detecting preheating in proto-clusters with Lyman-$\alpha$ Forest Tomography
• Prospects for Detection of Intracluster Gas Bulk Velocities Through the Sunyaev-Zel'dovich Effect
• Collisional interaction limits between dark matters and baryons in `cooling flow' clusters
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• Simulations of the merging cluster of galaxies Cygnus A
• On the X-ray emission from massive star clusters and their evolving superbubbles II. Detailed analytics and observational effects
• Testing General Relativity: new measurements of gravitational redshift in galaxy clusters
• Photometric Properties of Galaxy Population in the Cluster EIS 0048-2942 at z~0.64
• Investigation of Gravitational Lens Mass Models
• Dark Matter Profiles in Clusters of Galaxies: a Phenomenological Approach
• Gravitational Lensing by Galaxy Groups in the Hubble Deep Field
• A counter-image to the gravitational arc in Abell 1201: Evidence for IMF variations, or a $10^{10}$M${}_{\odot }$ black hole?
• Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
• Constraining Dark Energy From Splitting Angle Statistic of Strong Gravitational Lenses
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• Condensation of Galactic Cold Dark Matter
• Charged black hole surrounded by a galactic halo in de Sitter universe
• Cross-correlation between the soft X-ray background and SZ Sky
• Addressing via N-body simulations the distribution of the satellite tidal debris in the Milky Way environment
• Accurate Masses for Navarro-Frenk-White Dark Matter Haloes
• Maximum entropy distributions of dark matter in $\Lambda$CDM cosmology
• Cosmological Implications and Physical Properties of an X-Ray Flux-Limited Sample of Galaxy Clusters
• Physical modelling of galaxy clusters detected by Planck
• Fundamental Physics and Cosmology with TianQin
• The differential energy distribution of the universal density profile of dark halo
• X-ray surface brightness observations of galaxy clusters, cosmic opacity and the limits on the matter density parameter
• Effect of small scale density perturbations on the formation of dark matter halo profiles
• Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
• Constraints on the warm dark matter model from gravitational lensing
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• NGC 765 - A disturbed H I giant
• Central gas entropy excess as a direct evidence for AGN feedback in galaxy groups and clusters
• Magnetorotational instability in cool cores of galaxy clusters
• Profiles of dark-matter haloes at high redshift
• Intracluster Short Gamma-Ray Bursts by Compact Binary Mergers
• A Comparison of Simple Mass Estimators for Galaxy Clusters
• Temperature Structure and Mass-Temperature Scatter In Galaxy Clusters
• Angular momentum in cluster Spherical Collapse Model
• An expanded merger-tree description of cluster evolution
• Evolution of Low Mass Galactic Subhalos and Dependence on Concentration
• Improvements in the M-T relation and mass function and the measured Omega_m through clusters evolution
• On the Xray Luminosity - velocity dispersion relation of groups of galaxies
• Detecting the dark matter annihilation at the ground EAS detectors
• Catalog of Galaxy Morphology in Four Rich Clusters: Luminosity Evolution of Disk Galaxies at 0.33<z<0.83
• The density profiles of hot galactic halo gas
• A Gaia based photometric and kinematic analysis of the old open cluster King 11
• Weak Lensing analysis of Abell 2390 using short exposures
• Dynamical friction on cold fractal gas clouds,applications to disc formation
• Disk Galaxy Evolution Along the Hubble Sequence
• Cosmological Simulations with Scale-Free Initial Conditions I: Adiabatic Hydrodynamics
• Einasto profile as the halo model solution coupled to the depletion radius
• What Could be the Observational Signature of Dark Matter in Globular Clusters?
• Spherical accretion in giant elliptical galaxies: multi-transonicity, shocks, and implications on AGN feedback
• X-ray emission from RX J1720.1+2638 and Abell 267: a comparison between a fossil and a non-fossil system
• Perfect fluid dark matter: a viability test with galaxy rotation curves
• Interactions, Mergers and the Fundamental Mass Relations of Galaxies
• Redshift estimation of clusters by wavelet decomposition of their Sunyaev-Zel'dovich morphology
• Cosmological contribution from population III stars in ultracompact minihalos
• RX J1548.9+0851, a fossil cluster?
• On the abundance of gravitational arcs produced by submillimeter galaxies at radio and submm wavelengths
• Radial density and temperature profiles of the intracluster gas constructed jointly from the X-ray surface brightness measurement and the universal density profile
• Destruction of the central black hole gas reservoir through head-on galaxy collisions
• Scaling of the 1-halo terms with bias
• Comparison of physical and observational galaxy cluster modelling
• The Cosmological Mass Function with 1D Gravity
• Constraints on the Neutrino Mass from SZ Surveys
• The cluster abundance in cosmic string models for structure formation
• Numerical modelling of the lobes of radio galaxies -- Paper V: Universal Pressure Profile cluster atmospheres
• Hierarchical clustering and the baryon distribution in galaxy clusters
• Semi analytical description of formation of galaxies and clusters of galaxies
• Homeoidally striated density profiles: sequences of virial equilibrium configurations with constant anisotropy parameters
• Kinematical & Chemical Characteristics of the Thin and Thick Disks
• Effect of generic dark matter halo on transonic accretion onto galactic black holes
• Measurement of differential magnification
• The Wendelstein Weak Lensing (WWL) pathfinder: Accurate weak lensing masses for Planck clusters
• The abundance of lensing protoclusters
• Predicting the Non-Thermal Pressure in Galaxy Clusters
• Distinguishing dark matter halos with Extreme mass ratio inspirals
• Superheavy dark matter and ultrahigh energy cosmic rays
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• Detection of nonrandom patterns in cosmological gravitational clustering
• Galaxies with Supermassive Binary Black Holes: (II) A Model with Cuspy Galactic Density Profiles
• Soft X-ray excess of clusters: a thermal filament model, and the strong lensing of background galaxy groups
• The role of elliptic integrals in calculating the gravitational lensing of a charged Weyl black hole surrounded by plasma
• Optical Confirmation of X-ray selected Galaxy clusters from the Swift AGN and Cluster survey with MDM and Pan-STARRS Data (Paper III)
• The Jet Paths of Radio AGN and their Cluster Weather
• Resolving the jeans mass in hydrodynamic simulations of hierarchical clustering
• Population Studies of the Unidentified EGRET Sources
• A luminosity constraint on the origin of unidentified high energy sources
• Breaks in the X-ray spectra of high redshift blazars and the intervening medium
• A necessary condition for best fitting analytical to simulated density profiles in dark matter haloes
• The velocity field of collapsing spherical structures. Limitations of the spherical infall model in mass estimation
• Galaxies and Cluster of Galaxies as Peak Patches of the Density Field
• Ultra-High Energy Cosmic Rays: The Annihilation of Super-Heavy Relics
• Distribution Function of Dark Matter with Constant Anisotropy
• Galactic Escape Speeds in Mirror and Cold Dark Matter Models
• Predicting the Scaling Relations between the Dark Matter Halo Mass and Observables from Generalised Profiles II: Intracluster Gas Emission
• SZ power spectrum and cluster numbers from an extended merger-tree model
• Observational tests of the delta_c-M_vir relation in hierarchical clustering models
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• Scaling Relations in Dissipationless Spiral-like Galaxy Mergers
• Distribution Function in Center of Dark Matter Halo
• Holes within galaxies: the egg or the hen?
• Numerical modelling of the lobes of radio galaxies VI. Polarimetric simulations of universal pressure profile cluster atmospheres
• A new model for spherical galaxies and its distribution functions
• General relativistic quasi-spherical accretion in a dark matter halo
• A cellular automaton model of gravitational clustering
• Multi-transonic spherical-type flows around massive black holes: galactic potential induced standing isothermal shocks
• On the Size Evolution of a Galactic Disk in Hierarchical Merging of Cold Dark Matter Halos
• A short review on joint weak and strong cluster lens-mass reconstruction
• Numerical approaches to star formation and SuperNovae energy feedback in simulations of galaxy clusters
• Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison
• Chandra Study of the Massive and Distant Galaxy Cluster SDSS J0150-1005
• The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\mathrm{X}}$--$T$ relation of early-type galaxies
• Gravitational octree code performance evaluation on Volta GPU
• Universal Basic Mass Density inside Dark Matter Halos
• Weak gravitational flexion in various spacetimes: Exotic lenses and modified gravity
• Tidal Limit of Stellar Systems in Two-Power Density Models
• Understanding disk galaxy rotation velocities without dark matter contribution--a physical process for MOND?
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• Gravitational collapse and non-self similarity in the L-T relation