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WKP|Q116186250
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(WKP)Q116186250
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(OCoLC)Q116186250
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Thomas W. Jones
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American astronomer
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1
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iso5218
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670
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Author's 3D MHD interactions of jets with cluster media
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670
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Author's A Divergence‐free Upwind Code for Multidimensional Magnetohydrodynamic Flows
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670
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Author's A Multidimensional Code for Isothermal Magnetohydrodynamic Flows in Astrophysics
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670
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Author's Acoustic instability in cosmic ray mediated shocks
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670
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Author's Cluster Accretion Shocks as Possible Acceleration Sites for Ultra--High-Energy Protons below the Greisen Cutoff
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670
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Author's Computation of relativistic electron acceleration, transport and emissions in complex astrophysical flows
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670
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‡a
Author's Cosmic‐Ray Electrons in Groups and Clusters of Galaxies: Primary and Secondary Populations from a Numerical Cosmological Simulation
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670
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‡a
Author's Cosmic‐Ray Protons Accelerated at Cosmological Shocks and Their Impact on Groups and Clusters of Galaxies
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670
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Author's Cosmological Shock Waves and Their Role in the Large‐Scale Structure of the Universe
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670
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Author's Diffusive shock acceleration simulations of radio relics
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670
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Author's Effects of Cooling on the Propagation of Magnetized Jets
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670
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Author's Enhanced Cloud Disruption by Magnetic Field Interaction.
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670
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Author's Filaments in the southern giant lobe of Centaurus A: constraints on nature and origin from modelling and GMRT observations
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670
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‡a
Author's Hydrodynamics of Cloud Collisions in Two Dimensions: The Fate of Clouds in a Multiphase Medium
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670
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Author's Influence of Magnetic Fields on Pulsed, Radiative Jets
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670
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‡a
Author's INJECTION OF κ-LIKE SUPRATHERMAL PARTICLES INTO DIFFUSIVE SHOCK ACCELERATION
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670
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Author's Interactions between Radio Galaxies and Cluster Shocks. I. Jet Axes Aligned with Shock Normals
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670
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Author's Magnetohydrodynamics of Cloud Collisions in a Multiphase Interstellar Medium
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670
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Author's Model dust envelopes around late-type stars
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670
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Author's Numerical magetohydrodynamics in astrophysics: Algorithm and tests for one-dimensional flow`
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670
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Author's Numerical Magnetohydrodynamics in Astrophysics: Algorithm and Tests for Multidimensional Flow
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670
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Author's Numerical Study of Compressible Magnetohydrodynamic Turbulence in Two Dimensions
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670
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Author's Oblique magnetohydrodynamic cosmic-ray-modified shocks: Two-fluid numerical simulations
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670
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Author's On the Exchange of Kinetic and Magnetic Energy between Clouds and the Interstellar Medium
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670
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Author's Properties of Cosmic Shock Waves in Large‐Scale Structure Formation
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670
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Author's Radio Galaxy Zoo: discovery of a poor cluster through a giant wide-angle tail radio galaxy
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670
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Author's Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection
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670
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Author's Self-similar evolution of cosmic-ray modified shocks: the cosmic-ray spectrum
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670
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Author's Shock Acceleration Model for the Toothbrush Radio Relic
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670
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Author's Simulating Electron Transport and Synchrotron Emission in Radio Galaxies: Shock Acceleration and Synchrotron Aging in Axisymmetric Flows
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670
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Author's Simulating Electron Transport and Synchrotron Emission in Radio Galaxies: Shock Acceleration and Synchrotron Aging in Three‐Dimensional Flows
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670
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Author's Simulating magnetohydrodynamical flow with constrained transport and adaptive mesh refinement: algorithms and tests of the AstroBEAR code
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670
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Author's Simulations of nonthermal electron transport in multidimensional flows: application to radio galaxies
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670
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Author's Simulations of nonthermal electron transport in multidimensional flows: synthetic observations of radio galaxies
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670
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Author's Synthetic Observations of Simulated Radio Galaxies. I. Radio and X‐Ray Analysis
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670
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Author's The Effect of Cosmic‐Ray Diffusion on the Parker Instability
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670
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Author's The Magnetohydrodynamic Kelvin‐Helmholtz Instability: A Three‐dimensional Study of Nonlinear Evolution
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670
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Author's The Magnetohydrodynamic Kelvin-Helmholtz Instability: A Two-dimensional Numerical Study
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670
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Author's The Magnetohydrodynamic Kelvin‐Helmholtz Instability. III. The Role of Sheared Magnetic Field in Planar Flows
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670
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Author's The Magnetohydrodynamics of Supersonic Gas Clouds: MHD Cosmic Bullets and Wind‐swept Clumps
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670
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Author's The MHD Kelvin‐Helmholtz Instability. II. The Roles of Weak and Oblique Fields in Planar Flows
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670
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Author's The Propagation of Magnetocentrifugally Launched Jets. I
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670
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Author's The stability of cosmic-ray-dominated shocks - A secondary instability
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670
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Author's Three-dimensional Evolution of the Parker Instability under a Uniform Gravity
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670
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Author's Three‐dimensional Magnetohydrodynamic Numerical Simulations of Cloud‐Wind Interactions
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670
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Author's Three-dimensional simulations of bi-directed magnetohydrodynamic jets interacting with cluster environments
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670
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Author's Three‐dimensional Simulations of MHD Jet Propagation through Uniform and Stratified External Environments
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670
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Author's Three‐dimensional Simulations of the Parker Instability in a Uniformly Rotating Disk
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670
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Author's Time-dependent simulation of oblique MHD cosmic-ray shocks using the two-fluid model
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670
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Author's Turbulence and vorticity in Galaxy clusters generated by structure formation
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670
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Author's Vorticity, shocks, and magnetic fields in subsonic, ICM-like turbulence
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919
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effectofcosmicraydiffusionontheparkerinstability
‡A
The Effect of Cosmic‐Ray Diffusion on the Parker Instability
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1
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919
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simulationsofnonthermalelectrontransportinmultidimensionalflowssyntheticobservationsofradiogalaxies
‡A
Simulations of nonthermal electron transport in multidimensional flows: synthetic observations of radio galaxies
‡9
1
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919
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‡a
magnetohydrodynamickelvinhelmholtzinstability3theroleofshearedmagneticfieldinplanarflows
‡A
The Magnetohydrodynamic Kelvin‐Helmholtz Instability. III. The Role of Sheared Magnetic Field in Planar Flows
‡9
1
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919
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‡a
magnetohydrodynamicsofsupersonicgascloudsmhdcosmicbulletsandwindsweptclumps
‡A
The Magnetohydrodynamics of Supersonic Gas Clouds: MHD Cosmic Bullets and Wind‐swept Clumps
‡9
1
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919
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‡a
simulationsofnonthermalelectrontransportinmultidimensionalflowsapplicationtoradiogalaxies
‡A
Simulations of nonthermal electron transport in multidimensional flows: application to radio galaxies
‡9
1
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919
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‡a
mhdkelvinhelmholtzinstability2therolesofweakandobliquefieldsinplanarflows
‡A
The MHD Kelvin‐Helmholtz Instability. II. The Roles of Weak and Oblique Fields in Planar Flows
‡9
1
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919
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‡a
propagationofmagnetocentrifugallylaunchedjets1
‡A
The Propagation of Magnetocentrifugally Launched Jets. I
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1
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919
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simulatingmagnetohydrodynamicalflowwithconstrainedtransportandadaptivemeshrefinementalgorithmsandtestsoftheastrobearcode
‡A
Simulating magnetohydrodynamical flow with constrained transport and adaptive mesh refinement: algorithms and tests of the AstroBEAR code
‡9
1
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919
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‡a
stabilityofcosmicraydominatedshocksasecondaryinstability
‡A
The stability of cosmic-ray-dominated shocks - A secondary instability
‡9
1
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919
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‡a
3dimensionalevolutionoftheparkerinstabilityunderauniformgravity
‡A
Three-dimensional Evolution of the Parker Instability under a Uniform Gravity
‡9
1
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919
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‡a
3dimensionalmagnetohydrodynamicnumericalsimulationsofcloudwindinteractions
‡A
Three‐dimensional Magnetohydrodynamic Numerical Simulations of Cloud‐Wind Interactions
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1
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919
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simulatingelectrontransportandsynchrotronemissioninradiogalaxiesshockaccelerationandsynchrotronagingin3dimensionalflows
‡A
Simulating Electron Transport and Synchrotron Emission in Radio Galaxies: Shock Acceleration and Synchrotron Aging in Three‐Dimensional Flows
‡9
1
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919
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‡a
simulatingelectrontransportandsynchrotronemissioninradiogalaxiesshockaccelerationandsynchrotronaginginaxisymmetricflows
‡A
Simulating Electron Transport and Synchrotron Emission in Radio Galaxies: Shock Acceleration and Synchrotron Aging in Axisymmetric Flows
‡9
1
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919
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‡a
shockaccelerationmodelforthetoothbrushradiorelic
‡A
Shock Acceleration Model for the Toothbrush Radio Relic
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1
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919
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selfsimilarevolutionofcosmicraymodifiedshocksthecosmicrayspectrum
‡A
Self-similar evolution of cosmic-ray modified shocks: the cosmic-ray spectrum
‡9
1
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919
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‡a
3dimensionalsimulationsofbidirectedmagnetohydrodynamicjetsinteractingwithclusterenvironments
‡A
Three-dimensional simulations of bi-directed magnetohydrodynamic jets interacting with cluster environments
‡9
1
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919
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‡a
3dimensionalsimulationsofmhdjetpropagationthroughuniformandstratifiedexternalenvironments
‡A
Three‐dimensional Simulations of MHD Jet Propagation through Uniform and Stratified External Environments
‡9
1
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919
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‡a
3dimensionalsimulationsoftheparkerinstabilityinauniformlyrotatingdisk
‡A
Three‐dimensional Simulations of the Parker Instability in a Uniformly Rotating Disk
‡9
1
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919
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‡a
radiogalaxyzoohostgalaxiesandradiomorphologiesderivedfromvisualinspection
‡A
Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection
‡9
1
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919
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‡a
timedependentsimulationofobliquemhdcosmicrayshocksusingthe2fluidmodel
‡A
Time-dependent simulation of oblique MHD cosmic-ray shocks using the two-fluid model
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1
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919
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‡a
radiogalaxyzoodiscoveryofapoorclusterthroughagiantwideangletailradiogalaxy
‡A
Radio Galaxy Zoo: discovery of a poor cluster through a giant wide-angle tail radio galaxy
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1
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919
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‡a
turbulenceandvorticityingalaxyclustersgeneratedbystructureformation
‡A
Turbulence and vorticity in Galaxy clusters generated by structure formation
‡9
1
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919
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propertiesofcosmicshockwavesinlargescalestructureformation
‡A
Properties of Cosmic Shock Waves in Large‐Scale Structure Formation
‡9
1
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919
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vorticityshocksandmagneticfieldsinsubsonicicmliketurbulence
‡A
Vorticity, shocks, and magnetic fields in subsonic, ICM-like turbulence
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1
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919
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‡a
ontheexchangeofkineticandmagneticenergybetweencloudsandtheinterstellarmedium
‡A
On the Exchange of Kinetic and Magnetic Energy between Clouds and the Interstellar Medium
‡9
1
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919
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‡a
obliquemagnetohydrodynamiccosmicraymodifiedshocks2fluidnumericalsimulations
‡A
Oblique magnetohydrodynamic cosmic-ray-modified shocks: Two-fluid numerical simulations
‡9
1
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919
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‡a
numericalstudyofcompressiblemagnetohydrodynamicturbulencein2dimensions
‡A
Numerical Study of Compressible Magnetohydrodynamic Turbulence in Two Dimensions
‡9
1
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919
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‡a
numericalmagnetohydrodynamicsinastrophysicsalgorithmandtestsformultidimensionalflow
‡A
Numerical Magnetohydrodynamics in Astrophysics: Algorithm and Tests for Multidimensional Flow
‡9
1
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919
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‡a
numericalmagetohydrodynamicsinastrophysicsalgorithmandtestsfor1dimensionalflow
‡A
Numerical magetohydrodynamics in astrophysics: Algorithm and tests for one-dimensional flow`
‡9
1
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919
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‡a
modeldustenvelopesaroundlatetypestars
‡A
Model dust envelopes around late-type stars
‡9
1
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919
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‡a
magnetohydrodynamicsofcloudcollisionsinamultiphaseinterstellarmedium
‡A
Magnetohydrodynamics of Cloud Collisions in a Multiphase Interstellar Medium
‡9
1
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919
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|
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‡a
interactionsbetweenradiogalaxiesandclustershocks1jetaxesalignedwithshocknormals
‡A
Interactions between Radio Galaxies and Cluster Shocks. I. Jet Axes Aligned with Shock Normals
‡9
1
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919
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|
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‡a
injectionofκlikesuprathermalparticlesintodiffusiveshockacceleration
‡A
INJECTION OF κ-LIKE SUPRATHERMAL PARTICLES INTO DIFFUSIVE SHOCK ACCELERATION
‡9
1
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919
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‡a
influenceofmagneticfieldsonpulsedradiativejets
‡A
Influence of Magnetic Fields on Pulsed, Radiative Jets
‡9
1
|
919
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‡a
hydrodynamicsofcloudcollisionsin2dimensionsthefateofcloudsinamultiphasemedium
‡A
Hydrodynamics of Cloud Collisions in Two Dimensions: The Fate of Clouds in a Multiphase Medium
‡9
1
|
919
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|
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‡a
filamentsinthesoutherngiantlobeofcentaurusaconstraintsonnatureandoriginfrommodellingandgmrtobservations
‡A
Filaments in the southern giant lobe of Centaurus A: constraints on nature and origin from modelling and GMRT observations
‡9
1
|
919
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‡a
enhancedclouddisruptionbymagneticfieldinteraction
‡A
Enhanced Cloud Disruption by Magnetic Field Interaction.
‡9
1
|
919
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‡a
effectsofcoolingonthepropagationofmagnetizedjets
‡A
Effects of Cooling on the Propagation of Magnetized Jets
‡9
1
|
919
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‡a
diffusiveshockaccelerationsimulationsofradiorelics
‡A
Diffusive shock acceleration simulations of radio relics
‡9
1
|
919
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‡a
cosmologicalshockwavesandtheirroleinthelargescalestructureoftheuniverse
‡A
Cosmological Shock Waves and Their Role in the Large‐Scale Structure of the Universe
‡9
1
|
919
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‡a
cosmicrayprotonsacceleratedatcosmologicalshocksandtheirimpactongroupsandclustersofgalaxies
‡A
Cosmic‐Ray Protons Accelerated at Cosmological Shocks and Their Impact on Groups and Clusters of Galaxies
‡9
1
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919
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‡a
cosmicrayelectronsingroupsandclustersofgalaxiesprimaryandsecondarypopulationsfromanumericalcosmologicalsimulation
‡A
Cosmic‐Ray Electrons in Groups and Clusters of Galaxies: Primary and Secondary Populations from a Numerical Cosmological Simulation
‡9
1
|
919
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|
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‡a
computationofrelativisticelectronaccelerationtransportandemissionsincomplexastrophysicalflows
‡A
Computation of relativistic electron acceleration, transport and emissions in complex astrophysical flows
‡9
1
|
919
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|
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‡a
clusteraccretionshocksaspossibleaccelerationsitesforultrahighenergyprotonsbelowthegreisencutoff
‡A
Cluster Accretion Shocks as Possible Acceleration Sites for Ultra--High-Energy Protons below the Greisen Cutoff
‡9
1
|
919
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‡a
acousticinstabilityincosmicraymediatedshocks
‡A
Acoustic instability in cosmic ray mediated shocks
‡9
1
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919
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‡a
multidimensionalcodeforisothermalmagnetohydrodynamicflowsinastrophysics
‡A
A Multidimensional Code for Isothermal Magnetohydrodynamic Flows in Astrophysics
‡9
1
|
919
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‡a
divergencefreeupwindcodeformultidimensionalmagnetohydrodynamicflows
‡A
A Divergence‐free Upwind Code for Multidimensional Magnetohydrodynamic Flows
‡9
1
|
919
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‡a
3dmhdinteractionsofjetswithclustermedia
‡A
3D MHD interactions of jets with cluster media
‡9
1
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919
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‡a
syntheticobservationsofsimulatedradiogalaxies1radioand10rayanalysis
‡A
Synthetic Observations of Simulated Radio Galaxies. I. Radio and X‐Ray Analysis
‡9
1
|
919
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‡a
magnetohydrodynamickelvinhelmholtzinstabilitya2dimensionalnumericalstudy
‡A
The Magnetohydrodynamic Kelvin-Helmholtz Instability: A Two-dimensional Numerical Study
‡9
1
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919
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‡a
magnetohydrodynamickelvinhelmholtzinstabilitya3dimensionalstudyofnonlinearevolution
‡A
The Magnetohydrodynamic Kelvin‐Helmholtz Instability: A Three‐dimensional Study of Nonlinear Evolution
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1
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ISNI|0000000030634013
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996
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LC|no2010092600
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996
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NTA|068469160
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BIBSYS|12042573
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996
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SKMASNL|vtls009711421
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BNF|12736067
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CAOONL|ncf11661146
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LC|n 97005064
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LC|no 95004668
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ISNI|0000000077337606
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NUKAT|n 01091227
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CAOONL|ncf10203938
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NUKAT|n 2013059482
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LC|no2013097842
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LC|n 2011009709
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LC|n 92100400
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DNB|111937054X
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ISNI|0000000074926229
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LC|n 96110196
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ISNI|0000000052803236
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ISNI|0000000077926312
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BNF|17723844
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ISNI|0000000035407645
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J9U|987007392079905171
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LC|n 88002090
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BIBSYS|5007953
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LC|no2007036165
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ISNI|0000000049905557
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ISNI|0000000081922728
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DNB|1310450404
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996
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J9U|987007452536205171
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LC|no 89020359
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LC|n 87935413
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SUDOC|08412105X
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996
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ISNI|0000000425477972
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ISNI|0000000042786743
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RERO|A012512097
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DE633|pe30012569
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LC|no2017004144
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NUKAT|n 2016183766
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LC|n 94066340
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KRNLK|KAC200901375
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LC|n 98052172
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NTA|072942622
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LC|n 2002066702
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PLWABN|9810603690605606
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996
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LC|no2009052879
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ISNI|0000000065625547
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ISNI|0000000042076581
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CAOONL|ncf11587652
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LC|no2011042268
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NUKAT|n 2017171783
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N6I|vtls000274670
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996
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LC|n 90615994
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ISNI|0000000499157234
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ISNI|0000000033794784
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NTA|069489181
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ISNI|0000000075864146
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DNB|117655732
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996
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J9U|987012356658405171
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996
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N6I|vtls001093996
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996
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SUDOC|158417283
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996
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ISNI|0000000084353559
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‡2
ISNI|0000000446992914
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996
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ISNI|0000000095700499
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996
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LC|n 2012011670
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996
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RERO|A003430173
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996
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DNB|118895877
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996
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ISNI|0000000063050911
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SUDOC|257697365
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DNB|1055217134
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ISNI|0000000117706964
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SUDOC|135261759
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LC|no 98133577
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ISNI|0000000366566472
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996
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LNB|LNC10-000243791
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996
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PLWABN|9812830181705606
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996
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BAV|495_157142
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996
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BNF|17007469
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996
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LC|n 94098449
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LC|no 90015619
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LC|no2004049491
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996
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ISNI|0000000048050120
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LC|no2014084018
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996
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NTA|071632662
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996
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ISNI|0000000032982134
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996
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JPG|500068820
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DNB|1027274188
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996
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DNB|1205271694
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996
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ISNI|0000000055084273
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996
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LC|n 2002065655
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DBC|87097919156060
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996
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ISNI|0000000436101858
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DNB|138023867
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LC|no2011167214
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LC|nr 93025065
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996
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J9U|987007263536105171
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996
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ISNI|0000000080493503
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996
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LC|nr 92041162
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996
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CAOONL|ncf11671389
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996
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NTA|329323547
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996
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NII|DA13199752
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996
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DNB|130660159
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ISNI|0000000139074523
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996
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J9U|987007434614305171
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996
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J9U|987007458820805171
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996
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BIBSYS|13061144
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ISNI|0000000027100846
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LC|nb2012004554
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NTA|115781463
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BNF|13758006
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996
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PLWABN|9810612870805606
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996
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LC|n 93079805
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ISNI|0000000496318709
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J9U|987007465335705171
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996
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JPG|500008222
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996
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DNB|1157356303
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996
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BAV|495_134754
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996
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N6I|vtls000069001
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996
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LC|n 2001034229
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LC|n 2006003265
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LC|no2009110105
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996
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BNF|12523663
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ISNI|0000000360064201
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996
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NTA|251935930
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996
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BIBSYS|4073514
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LC|nr 90002050
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N6I|vtls001351746
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N6I|vtls000102324
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996
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LC|nb2012012264
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996
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J9U|987007461859105171
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996
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RERO|A017589660
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RERO|A022788736
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996
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LC|nr 92035291
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996
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RERO|A022894679
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996
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NLA|000035917661
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996
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LC|nr2006010979
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LC|n 86827404
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LC|nb2009010681
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NTA|251960153
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DNB|123618045
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LC|n 99836097
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996
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BIBSYS|90506848
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SIMACOB|22867043
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N6I|vtls000042817
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996
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BNE|XX5783094
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NII|DA1197184X
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996
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NSK|000302444
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BNC|981058614490706706
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996
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DNB|1271654725
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LC|no2008159402
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ISNI|0000000036294830
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JPG|500091096
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BIBSYS|90518254
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996
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J9U|987007339755305171
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996
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ISNI|0000000110848855
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LC|n 79137080
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ISNI|0000000118273179
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BIBSYS|6054901
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N6I|vtls001380162
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996
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LC|n 85336673
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BIBSYS|13068022
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996
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LC|no2009194790
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LC|no2019123343
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LC|n 88119202
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DNB|1043671870
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ISNI|0000000044694076
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LC|no2009159103
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LC|n 77000909
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DNB|1282398253
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J9U|987007426231305171
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LC|no2010116607
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BIBSYS|90102761
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ISNI|000000010776620X
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LC|no2003067306
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LC|no2009188259
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BNF|13532046
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NTA|440242568
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DNB|173236367
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LC|nr 98037320
|
996
|
|
|
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NII|DA07242132
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996
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|
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NTA|074759175
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997
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‡a
0 0 lived 0 0
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1
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