Publication data of Ostriker, Eve C.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025010002000300040005000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250204060801000246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025010203040
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe CO-H2 Conversion Factor in Disc Galaxies and MergersMagnetorotationally-driven galactic turbulence and the formation of giant molecular cloudsMagnetorotationally-driven galactic turbulence and the formation of giant m…Three-dimensional simulations of parker, magneto-jeans, and swing instabilities in shearing galactic gas disksThree-dimensional simulations of parker, magneto-jeans, and swing instabiliti…Analysis of clumps in molecular cloud models: Mass spectrum, shapes, alignment and rotationAnalysis of clumps in molecular cloud models: Mass spectrum, shapes, align…Hot one temperature accretion flows around black holesFormation of spiral-arm spurs and bound clouds in vertically stratified galactic gas disksFormation of spiral-arm spurs and bound clouds in vertically stratified galacti…Can nonlinear hydromagnetic waves support a selfgravitating cloud?Formation and fragmentation of gaseous spurs in spiral galaxiesAmplification, saturation, and q thresholds for runaway: Growth of selfgravitating structures in models of magnetized galactic gas disksAmplification, saturation, and q thresholds for runaway: Growth of selfgravita…The State of the Gas and the Relation Between Gas and Star Formation at Low Metallicity: the Small Magellanic CloudThe State of the Gas and the Relation Between Gas and Star Formation at Lo…Regulation of Star Formation Rates in Multiphase Galactic Disks: a Thermal/Dynamical Equilibrium ModelRegulation of Star Formation Rates in Multiphase Galactic Disks: a Thermal/D…Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven TurbulenceMaximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-D…A General Model for the CO-H2 Conversion Factor in Galaxies with Applications to the Star Formation LawA General Model for the CO-H2 Conversion Factor in Galaxies with Application…Kinetic and structural evolution of selfgravitating, magnetized clouds: 2.5-dimensional simulations of decaying turbulenceKinetic and structural evolution of selfgravitating, magnetized clouds: 2.5-di…Dissipation in compressible MHD turbulenceDensity, velocity, and magnetic field structure in turbulent molecular cloud modelsDensity, velocity, and magnetic field structure in turbulent molecular cloud …Dynamical friction in a gaseous mediumMagnetocentrifugally driven flows from young stars and disks. 1. A generalized modelMagnetocentrifugally driven flows from young stars and disks. 1. A generalized modelMagnetocentrifugally driven flows from young stars and disks. 1. A generaliz…Theory of Star Formation1995200020052010201520202025010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The CO-H2 Conversion Factor in Disc Galaxies and MergersMagnetorotationally-driven galactic turbulence and the formation of giant molecular cloudsMagnetorotationally-driven galactic turbulence and the formation of giant m…Three-dimensional simulations of parker, magneto-jeans, and swing instabilities in shearing galactic gas disksThree-dimensional simulations of parker, magneto-jeans, and swing instabiliti…Analysis of clumps in molecular cloud models: Mass spectrum, shapes, alignment and rotationAnalysis of clumps in molecular cloud models: Mass spectrum, shapes, align…Hot one temperature accretion flows around black holesFormation of spiral-arm spurs and bound clouds in vertically stratified galactic gas disksFormation of spiral-arm spurs and bound clouds in vertically stratified galacti…Can nonlinear hydromagnetic waves support a selfgravitating cloud?Formation and fragmentation of gaseous spurs in spiral galaxiesAmplification, saturation, and q thresholds for runaway: Growth of selfgravitating structures in models of magnetized galactic gas disksAmplification, saturation, and q thresholds for runaway: Growth of selfgravita…The State of the Gas and the Relation Between Gas and Star Formation at Low Metallicity: the Small Magellanic CloudThe State of the Gas and the Relation Between Gas and Star Formation at Lo…Regulation of Star Formation Rates in Multiphase Galactic Disks: a Thermal/Dynamical Equilibrium ModelRegulation of Star Formation Rates in Multiphase Galactic Disks: a Thermal/D…Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven TurbulenceMaximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-D…A General Model for the CO-H2 Conversion Factor in Galaxies with Applications to the Star Formation LawA General Model for the CO-H2 Conversion Factor in Galaxies with Application…Kinetic and structural evolution of selfgravitating, magnetized clouds: 2.5-dimensional simulations of decaying turbulenceKinetic and structural evolution of selfgravitating, magnetized clouds: 2.5-di…Dissipation in compressible MHD turbulenceDensity, velocity, and magnetic field structure in turbulent molecular cloud modelsDensity, velocity, and magnetic field structure in turbulent molecular cloud …Dynamical friction in a gaseous mediumMagnetocentrifugally driven flows from young stars and disks. 1. A generalized modelMagnetocentrifugally driven flows from young stars and disks. 1. A generalized modelMagnetocentrifugally driven flows from young stars and disks. 1. A generaliz…Theory of Star Formation19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250100200300400500