Publication data of Fujita, Yutaka: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025050010001500200025003000
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-citaion199520002005201020152020202505101520253035
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestSlow Diffusion of Cosmic-Rays around a Supernova RemnantSuzaku observations of the Hydra A cluster out to the virial radiusDiscovery of a new subparsec counterjet in NGC 1275: the inclination angle and the environmentDiscovery of a new subparsec counterjet in NGC 1275: the inclination angle …Chandra observations of the disruption of the cool core in abell 133Suzaku observations of Abell 1835 outskirts: Deviation from hydrostatic equilibriumSuzaku observations of Abell 1835 outskirts: Deviation from hydrostatic equil…Is galactic star formation activity increased during cluster mergers?Nonthermal emission from accreting and merging clusters of galaxiesNonthermal Emission Associated with Strong AGN Outbursts at the Centers of Galaxy ClustersNonthermal Emission Associated with Strong AGN Outbursts at the Centers o…Suzaku Observation of the Ophiuchus Galaxy Cluster: One of the Hottest Cool Core ClustersSuzaku Observation of the Ophiuchus Galaxy Cluster: One of the Hottest Cool…Strong 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…High Metallicity of the X-Ray Gas up to the Virial Radius of a Binary Cluster of Galaxies: Evidence of Galactic Superwinds at High-RedshiftHigh Metallicity of the X-Ray Gas up to the Virial Radius of a Binary Cluster of …Molecular Clouds as a Probe of Cosmic-Ray Acceleration in a Supernova RemnantMolecular Clouds as a Probe of Cosmic-Ray Acceleration in a Supernova Remn…Quantitative estimates of environmental effects on the star formation rate of disk galaxies in clusters of galaxiesQuantitative estimates of environmental effects on the star formation rate of …Can we explain AMS-02 antiproton and positron excesses simultaneously by nearby supernovae without pulsars or dark matter?Can we explain AMS-02 antiproton and positron excesses simultaneously by …Pre-processing of galaxies before entering a clusterEffects of ram-pressure from intracluster medium on the star formation rate of disk galaxies in clusters of galaxiesEffects of ram-pressure from intracluster medium on the star formation rate …Is the PAMELA anomaly caused by the supernova explosions near the Earth?Nonthermal emissions from particles accelerated by turbulence in clusters of galaxiesNonthermal emissions from particles accelerated by turbulence in clusters of…The Morphology - density relation in the SDSS1995200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Slow Diffusion of Cosmic-Rays around a Supernova RemnantSuzaku observations of the Hydra A cluster out to the virial radiusDiscovery of a new subparsec counterjet in NGC 1275: the inclination angle and the environmentDiscovery of a new subparsec counterjet in NGC 1275: the inclination angle …Chandra observations of the disruption of the cool core in abell 133Suzaku observations of Abell 1835 outskirts: Deviation from hydrostatic equilibriumSuzaku observations of Abell 1835 outskirts: Deviation from hydrostatic equil…Is galactic star formation activity increased during cluster mergers?Nonthermal emission from accreting and merging clusters of galaxiesNonthermal Emission Associated with Strong AGN Outbursts at the Centers of Galaxy ClustersNonthermal Emission Associated with Strong AGN Outbursts at the Centers o…Suzaku Observation of the Ophiuchus Galaxy Cluster: One of the Hottest Cool Core ClustersSuzaku Observation of the Ophiuchus Galaxy Cluster: One of the Hottest Cool…Strong 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…High Metallicity of the X-Ray Gas up to the Virial Radius of a Binary Cluster of Galaxies: Evidence of Galactic Superwinds at High-RedshiftHigh Metallicity of the X-Ray Gas up to the Virial Radius of a Binary Cluster of …Molecular Clouds as a Probe of Cosmic-Ray Acceleration in a Supernova RemnantMolecular Clouds as a Probe of Cosmic-Ray Acceleration in a Supernova Remn…Quantitative estimates of environmental effects on the star formation rate of disk galaxies in clusters of galaxiesQuantitative estimates of environmental effects on the star formation rate of …Can we explain AMS-02 antiproton and positron excesses simultaneously by nearby supernovae without pulsars or dark matter?Can we explain AMS-02 antiproton and positron excesses simultaneously by …Pre-processing of galaxies before entering a clusterEffects of ram-pressure from intracluster medium on the star formation rate of disk galaxies in clusters of galaxiesEffects of ram-pressure from intracluster medium on the star formation rate …Is the PAMELA anomaly caused by the supernova explosions near the Earth?Nonthermal emissions from particles accelerated by turbulence in clusters of galaxiesNonthermal emissions from particles accelerated by turbulence in clusters of…The Morphology - density relation in the SDSS19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025050100150200