Publication data of Arnett, W.David: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion197019801990200020102020010002000300040005000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19701980199020002010202002040608010001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19701980199020002010202005101520253035
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestDynamics of circumstellar disksObservational tests and predictive stellar evolution. 2. Non-standard modelsTurbulent Cells in Stars: I. Fluctuations in Kinetic Energy and LuminosityTurbulent Convection in Stellar Interiors. II. The Velocity FieldActive carbon and oxygen shell burning hydrodynamicsTwo-dimensional hydrodynamics of pre-core collapse: oxygen shell burningThe Late Behavior of Supernova {SN1987A}Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach 3, gamma = 5/3Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach…Neutrino Mass Limits From Sn1987aConstraints on the progenitor of cassiopeia aThe Three Dimensional Evolution to Core Collapse of a Massive StarNeutrino Trapping During Gravitational Collapse of StarsTowards Realistic Progenitors of Core-Collapse SupernovaeTurbulent Convection in Stellar Interiors. 1. Hydrodynamic SimulationPreparing for an Explosion: Hydrodynamic Instabilities and Turbulence in PresupernovaePreparing for an Explosion: Hydrodynamic Instabilities and Turbulence in Pres…A Microscopic Interpretation of Neutron Star StructureThe Evolution and fate of Very Massive ObjectsSUPERNOVA SN1987AType I supernovae. I - Analytic solutions for the early part of the light curve197019801990200020102020010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Dynamics of circumstellar disksObservational tests and predictive stellar evolution. 2. Non-standard modelsTurbulent Cells in Stars: I. Fluctuations in Kinetic Energy and LuminosityTurbulent Convection in Stellar Interiors. II. The Velocity FieldActive carbon and oxygen shell burning hydrodynamicsTwo-dimensional hydrodynamics of pre-core collapse: oxygen shell burningThe Late Behavior of Supernova {SN1987A}Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach 3, gamma = 5/3Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach…Neutrino Mass Limits From Sn1987aConstraints on the progenitor of cassiopeia aThe Three Dimensional Evolution to Core Collapse of a Massive StarNeutrino Trapping During Gravitational Collapse of StarsTowards Realistic Progenitors of Core-Collapse SupernovaeTurbulent Convection in Stellar Interiors. 1. Hydrodynamic SimulationPreparing for an Explosion: Hydrodynamic Instabilities and Turbulence in PresupernovaePreparing for an Explosion: Hydrodynamic Instabilities and Turbulence in Pres…A Microscopic Interpretation of Neutron Star StructureThe Evolution and fate of Very Massive ObjectsSUPERNOVA SN1987AType I supernovae. I - Analytic solutions for the early part of the light curve1970198019902000201020200255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average197019801990200020102020050100150200250300350