Publication data of Wada, Keiichi: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion199520002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1995200020052010201520202025030609012015002.557.51012.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe three-dimensional structure of a massive gas disk in the galactic central regionThe three-dimensional structure of a massive gas disk in the galactic central …Tidal disruption of dark matter halos around proto-globular clustersInstabilities of spiral shocks 1: Onset of wiggle instability and its mechanismFeedback from the first supernovae in protogalaxies: The Fate of the generated metalsFeedback from the first supernovae in protogalaxies: The Fate of the generat…Comparison of nuclear starburst luminosities between Seyfert 1 and 2 galaxies based on near-infrared spectroscopyComparison of nuclear starburst luminosities between Seyfert 1 and 2 galaxi…Radiation Hydrodynamic Simulations of Line-Driven Disk Winds for Ultra Fast OutflowsRadiation Hydrodynamic Simulations of Line-Driven Disk Winds for Ultra Fast …Interplay between Stellar Spirals and the ISM in Galactic DisksRadiation-driven Fountain and Origin of Torus around Active Galactic NucleiToward First-Principle Simulations of Galaxy Formation: II. Shock-Induced Starburst at a Collision Interface During the First Encounter of Interacting GalaxiesToward First-Principle Simulations of Galaxy Formation: II. Shock-Induced Sta…The global structure and evolution of a selfgravitating multi-phase interstellar medium in a galactic diskThe global structure and evolution of a selfgravitating multi-phase interstellar…Coevolution of Supermassive Black Holes and Circumnuclear DisksStrong turbulence in the cool cores of galaxy clusters: Can tsunamis solve the cooling flow problem?Strong turbulence in the cool cores of galaxy clusters: Can tsunamis solve th…Formation of cavities, filaments, and clumps by the nonlinear development of thermal and gravitational instabilities in the interstellar medium under stellar feedbackFormation of cavities, filaments, and clumps by the nonlinear development o…Toward first-principle simulations of galaxy formation: I. How should we choose star formation criteria in high-resolution simulations of disk galaxies?Toward first-principle simulations of galaxy formation: I. How should we choo…Molecular Gas Disk Structures around AGNsGravity-driven turbulence in galactic disksDensity structure of the interstellar medium and the star formation rate in galactic disksDensity structure of the interstellar medium and the star formation rate in g…Obscuring material around seyfert nuclei with starburstsNumerical Models of the Multiphase Interstellar Matter with Stellar Energy Feedback on a Galactic ScaleNumerical Models of the Multiphase Interstellar Matter with Stellar Energy Fe…199520002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The three-dimensional structure of a massive gas disk in the galactic central regionThe three-dimensional structure of a massive gas disk in the galactic central …Tidal disruption of dark matter halos around proto-globular clustersInstabilities of spiral shocks 1: Onset of wiggle instability and its mechanismFeedback from the first supernovae in protogalaxies: The Fate of the generated metalsFeedback from the first supernovae in protogalaxies: The Fate of the generat…Comparison of nuclear starburst luminosities between Seyfert 1 and 2 galaxies based on near-infrared spectroscopyComparison of nuclear starburst luminosities between Seyfert 1 and 2 galaxi…Radiation Hydrodynamic Simulations of Line-Driven Disk Winds for Ultra Fast OutflowsRadiation Hydrodynamic Simulations of Line-Driven Disk Winds for Ultra Fast …Interplay between Stellar Spirals and the ISM in Galactic DisksRadiation-driven Fountain and Origin of Torus around Active Galactic NucleiToward First-Principle Simulations of Galaxy Formation: II. Shock-Induced Starburst at a Collision Interface During the First Encounter of Interacting GalaxiesToward First-Principle Simulations of Galaxy Formation: II. Shock-Induced Sta…The global structure and evolution of a selfgravitating multi-phase interstellar medium in a galactic diskThe global structure and evolution of a selfgravitating multi-phase interstellar…Coevolution of Supermassive Black Holes and Circumnuclear DisksStrong turbulence in the cool cores of galaxy clusters: Can tsunamis solve the cooling flow problem?Strong turbulence in the cool cores of galaxy clusters: Can tsunamis solve th…Formation of cavities, filaments, and clumps by the nonlinear development of thermal and gravitational instabilities in the interstellar medium under stellar feedbackFormation of cavities, filaments, and clumps by the nonlinear development o…Toward first-principle simulations of galaxy formation: I. How should we choose star formation criteria in high-resolution simulations of disk galaxies?Toward first-principle simulations of galaxy formation: I. How should we choo…Molecular Gas Disk Structures around AGNsGravity-driven turbulence in galactic disksDensity structure of the interstellar medium and the star formation rate in galactic disksDensity structure of the interstellar medium and the star formation rate in g…Obscuring material around seyfert nuclei with starburstsNumerical Models of the Multiphase Interstellar Matter with Stellar Energy Feedback on a Galactic ScaleNumerical Models of the Multiphase Interstellar Matter with Stellar Energy Fe…19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025050100150200