Publication data of Youdin, Andrew N.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2000200520102015202020250250500750100012501500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200020052010201520202025081624324001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20002005201020152020202505101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestPlanetesimal formation without thresholds. 2. gravitational instability of solids in turbulent protoplanetary disksPlanetesimal formation without thresholds. 2. gravitational instability of solids…Planetesimal formation without thresholds. 1. dissipative gravitational instabilities and particle stirring by turbulencePlanetesimal formation without thresholds. 1. dissipative gravitational instabil…On the Formation of Planetesimals via Secular Gravitational Instabilities with Turbulent StirringOn the Formation of Planetesimals via Secular Gravitational Instabilities with T…From Grains to PlanetesimalsFormation of Kuiper Belt Binaries by Gravitational CollapseThe Mechanical Greenhouse: Burial of Heat by Turbulence in Hot Jupiter AtmospheresThe Mechanical Greenhouse: Burial of Heat by Turbulence in Hot Jupiter Atmo…The Exoplanet Census: A General Method, Applied to KeplerForming Planetesimals in Solar and Extrasolar NebulaeParticle Stirring in Turbulent Gas Disks: Including Orbital OscillationsProtoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical MethodsProtoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Ev…Protoplanetary Disk Turbulence Driven by the Streaming Instability: Non-Linear Saturation and Particle ConcentrationProtoplanetary Disk Turbulence Driven by the Streaming Instability: Non-Line…Particle Clumping in Protoplanetary Disks Depends Strongly on MetallicityParticle pile-ups and planetesimal formationThe Runts of the Litter: Why planets formed through gravitational instability can only be failed binary starsThe Runts of the Litter: Why planets formed through gravitational instability …Zonal Flows and Long-Lived Axisymmetric Pressure Bumps in Magnetorotational TurbulenceZonal Flows and Long-Lived Axisymmetric Pressure Bumps in Magnetorotatio…Limits on spin - mass couplings within the axion windowStreaming instabilities in protoplanetary disksPlanetesimal formation by gravitational instabilityRapid planetesimal formation in turbulent circumstellar discs2000200520102015202020250250500750100012501500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Planetesimal formation without thresholds. 2. gravitational instability of solids in turbulent protoplanetary disksPlanetesimal formation without thresholds. 2. gravitational instability of solids…Planetesimal formation without thresholds. 1. dissipative gravitational instabilities and particle stirring by turbulencePlanetesimal formation without thresholds. 1. dissipative gravitational instabil…On the Formation of Planetesimals via Secular Gravitational Instabilities with Turbulent StirringOn the Formation of Planetesimals via Secular Gravitational Instabilities with T…From Grains to PlanetesimalsFormation of Kuiper Belt Binaries by Gravitational CollapseThe Mechanical Greenhouse: Burial of Heat by Turbulence in Hot Jupiter AtmospheresThe Mechanical Greenhouse: Burial of Heat by Turbulence in Hot Jupiter Atmo…The Exoplanet Census: A General Method, Applied to KeplerForming Planetesimals in Solar and Extrasolar NebulaeParticle Stirring in Turbulent Gas Disks: Including Orbital OscillationsProtoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical MethodsProtoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Ev…Protoplanetary Disk Turbulence Driven by the Streaming Instability: Non-Linear Saturation and Particle ConcentrationProtoplanetary Disk Turbulence Driven by the Streaming Instability: Non-Line…Particle Clumping in Protoplanetary Disks Depends Strongly on MetallicityParticle pile-ups and planetesimal formationThe Runts of the Litter: Why planets formed through gravitational instability can only be failed binary starsThe Runts of the Litter: Why planets formed through gravitational instability …Zonal Flows and Long-Lived Axisymmetric Pressure Bumps in Magnetorotational TurbulenceZonal Flows and Long-Lived Axisymmetric Pressure Bumps in Magnetorotatio…Limits on spin - mass couplings within the axion windowStreaming instabilities in protoplanetary disksPlanetesimal formation by gravitational instabilityRapid planetesimal formation in turbulent circumstellar discs2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200250300