Publication data of Goodwin, Simon P.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion198519901995200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19851990199520002005201020152020202502040608010002.557.51012.5
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe dynamical evolution of fractal star clusters: The Survival of substructureThe formation of very wide binaries during the star cluster dissolution phaseDo O-stars form in isolation?An Idealized pulsar magnetosphere: The Relativistic force-free approximationSimulating star formation in molecular cores. 2. The Effects of different levels of turbulenceSimulating star formation in molecular cores. 2. The Effects of different levels…The initial conditions of young globular clusters in the lmcThe SAMI Galaxy Survey: First detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxiesThe SAMI Galaxy Survey: First detection of a transition in spin orientation wit…Limits on the primordial stellar multiplicityIntermediate to low-mass stellar content of Westerlund 1Radiative transfer and the energy equation in SPH simulations of star formationRadiative transfer and the energy equation in SPH simulations of star formati…On mini-halo encounters with starsResidual gas expulsion from young globular clustersDynamical mass segregation on a very short timescaleSimulating star formation in molecular cloud cores. 1. The Influence of low levels of turbulence on fragmentation and multiplicitySimulating star formation in molecular cloud cores. 1. The Influence of low le…Physical parameters of the high-mass X-ray binary 4U1700-37Evidence for the strong effect of gas removal on the internal dynamics of young stellar clustersEvidence for the strong effect of gas removal on the internal dynamics of yo…On the massive stellar population of the super star cluster Westerlund 1Gas expulsion and the destruction of massive young clustersThe R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limitThe R136 star cluster hosts several stars whose individual masses greatly ex…198519901995200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The dynamical evolution of fractal star clusters: The Survival of substructureThe formation of very wide binaries during the star cluster dissolution phaseDo O-stars form in isolation?An Idealized pulsar magnetosphere: The Relativistic force-free approximationSimulating star formation in molecular cores. 2. The Effects of different levels of turbulenceSimulating star formation in molecular cores. 2. The Effects of different levels…The initial conditions of young globular clusters in the lmcThe SAMI Galaxy Survey: First detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxiesThe SAMI Galaxy Survey: First detection of a transition in spin orientation wit…Limits on the primordial stellar multiplicityIntermediate to low-mass stellar content of Westerlund 1Radiative transfer and the energy equation in SPH simulations of star formationRadiative transfer and the energy equation in SPH simulations of star formati…On mini-halo encounters with starsResidual gas expulsion from young globular clustersDynamical mass segregation on a very short timescaleSimulating star formation in molecular cloud cores. 1. The Influence of low levels of turbulence on fragmentation and multiplicitySimulating star formation in molecular cloud cores. 1. The Influence of low le…Physical parameters of the high-mass X-ray binary 4U1700-37Evidence for the strong effect of gas removal on the internal dynamics of young stellar clustersEvidence for the strong effect of gas removal on the internal dynamics of yo…On the massive stellar population of the super star cluster Westerlund 1Gas expulsion and the destruction of massive young clustersThe R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limitThe R136 star cluster hosts several stars whose individual masses greatly ex…1985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1985199019952000200520102015202020250100200300400