Publication data of Ruffert, M.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1995200020052010201520202025012243648600246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestSimulations of galactic winds and starbursts in galaxy clustersThree-dimensional hydrodynamic bondi-hoyle accretion. v. specific heat ratio 1.01, nearly isothermal flowThree-dimensional hydrodynamic bondi-hoyle accretion. v. specific heat ratio…Can neutrinos from neutron star mergers power gamma-ray bursts?A Fresh look at the unstable simulations of Bondi-Hoyle-Lyttleton accretionNon-axisymmetric wind-accretion simulations I. velocity gradients of 3% and 20% over one accretion radiusNon-axisymmetric wind-accretion simulations I. velocity gradients of 3% and …Enrichment of the ICM of galaxy clusters due to ram-pressure strippingThree-dimensional simulations of non-stationary accretion by remnant black holes of compact object mergersThree-dimensional simulations of non-stationary accretion by remnant black …Hydrodynamical 3-D Bondi-Hoyle accretion. 1. Code validation, stationary accretorHydrodynamical 3-D Bondi-Hoyle accretion. 1. Code validation, stationary acc…Non-stationary hyperaccretion of stellar - mass black holes in three dimensions: Torus evolution and neutrino emissionNon-stationary hyperaccretion of stellar - mass black holes in three dimensio…Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach 3, gamma = 5/3Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach…Non-axisymmetric wind-accretion simulations. 2. Density gradientsSimulations of non-axisymmetric rotational core collapseColliding neutron stars: Gravitational waves, neutrino emission, and gamma-ray burstsColliding neutron stars: Gravitational waves, neutrino emission, and gamma-r…Coalescing neutron stars - a step towards physical models. 3. Improved numerics and different neutron star masses and spinsCoalescing neutron stars - a step towards physical models. 3. Improved num…r-Process Nucleosynthesis in Hot Accretion Disk Flows from Black Hole - Neutron Star Mergersr-Process Nucleosynthesis in Hot Accretion Disk Flows from Black Hole - Neutr…Black hole: Neutron star mergers as central engines of gamma-ray burstsGamma-ray bursts from accreting black holes in neutron star mergersCoalescing neutron stars: A Step towards physical models. 1: Hydrodynamic evolution and gravitational wave emissionCoalescing neutron stars: A Step towards physical models. 1: Hydrodynamic …Coalescing neutron stars: A Step towards physical models. 2. Neutrino emission, neutron tori, and gamma-ray burstsCoalescing neutron stars: A Step towards physical models. 2. Neutrino emissi…1995200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Simulations of galactic winds and starbursts in galaxy clustersThree-dimensional hydrodynamic bondi-hoyle accretion. v. specific heat ratio 1.01, nearly isothermal flowThree-dimensional hydrodynamic bondi-hoyle accretion. v. specific heat ratio…Can neutrinos from neutron star mergers power gamma-ray bursts?A Fresh look at the unstable simulations of Bondi-Hoyle-Lyttleton accretionNon-axisymmetric wind-accretion simulations I. velocity gradients of 3% and 20% over one accretion radiusNon-axisymmetric wind-accretion simulations I. velocity gradients of 3% and …Enrichment of the ICM of galaxy clusters due to ram-pressure strippingThree-dimensional simulations of non-stationary accretion by remnant black holes of compact object mergersThree-dimensional simulations of non-stationary accretion by remnant black …Hydrodynamical 3-D Bondi-Hoyle accretion. 1. Code validation, stationary accretorHydrodynamical 3-D Bondi-Hoyle accretion. 1. Code validation, stationary acc…Non-stationary hyperaccretion of stellar - mass black holes in three dimensions: Torus evolution and neutrino emissionNon-stationary hyperaccretion of stellar - mass black holes in three dimensio…Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach 3, gamma = 5/3Hydrodynamical 3-D Bondi-Hoyle accretion. 2. Homogeneous medium, mach…Non-axisymmetric wind-accretion simulations. 2. Density gradientsSimulations of non-axisymmetric rotational core collapseColliding neutron stars: Gravitational waves, neutrino emission, and gamma-ray burstsColliding neutron stars: Gravitational waves, neutrino emission, and gamma-r…Coalescing neutron stars - a step towards physical models. 3. Improved numerics and different neutron star masses and spinsCoalescing neutron stars - a step towards physical models. 3. Improved num…r-Process Nucleosynthesis in Hot Accretion Disk Flows from Black Hole - Neutron Star Mergersr-Process Nucleosynthesis in Hot Accretion Disk Flows from Black Hole - Neutr…Black hole: Neutron star mergers as central engines of gamma-ray burstsGamma-ray bursts from accreting black holes in neutron star mergersCoalescing neutron stars: A Step towards physical models. 1: Hydrodynamic evolution and gravitational wave emissionCoalescing neutron stars: A Step towards physical models. 1: Hydrodynamic …Coalescing neutron stars: A Step towards physical models. 2. Neutrino emission, neutron tori, and gamma-ray burstsCoalescing neutron stars: A Step towards physical models. 2. Neutrino emissi…19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250255075100125150