Publication data of Miralles, Jose A.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1990199520002005201020152020202501000200030004000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1990199520002005201020152020202501530456075012345
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1990199520002005201020152020202505101520253035
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestA new code for the Hall-driven magnetic evolution of neutron starsThe relevance of ambipolar diffusion for neutron star evolutionPopulation synthesis of isolated neutron stars with magneto-rotational evolution – II. From radio-pulsars to magnetarsPopulation synthesis of isolated neutron stars with magneto-rotational evoluti…A new spherically symmetric general relativistic hydrodynamical codeAnisotropic thermal emission from magnetized neutron starsEvidence for Heating of Neutron Stars by Magnetic Field DecayConstraining the GRB-magnetar model by means of the Galactic pulsar populationConstraining the GRB-magnetar model by means of the Galactic pulsar popul…The impact of magnetic field on the thermal evolution of neutron starsSpectral evolution of superluminal components in parsec-scale jetsPopulation synthesis of isolated Neutron Stars with magneto-rotational evolutionPopulation synthesis of isolated Neutron Stars with magneto-rotational evolut…Evolution of protoneutron stars with kaon condensatesNumerical relativistic hydrodynamics: Local characteristic approachPopulation synthesis studies of isolated neutron stars with magnetic field decayPopulation synthesis studies of isolated neutron stars with magnetic field dec…2D Cooling of Magnetized Neutron StarsNumerical 3+1 general relativistic magnetohydrodynamics: A Local characteristic approachNumerical 3+1 general relativistic magnetohydrodynamics: A Local characte…Magneto--thermal evolution of neutron starsNumerical {3+1} General Relativistic Hydrodynamics: A Local Characteristic ApproachNumerical {3+1} General Relativistic Hydrodynamics: A Local Characteristic …Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution modelsUnifying the observational diversity of isolated neutron stars via magneto-the…Evolution of protoneutron stars1990199520002005201020152020202501000200030004000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)A new code for the Hall-driven magnetic evolution of neutron starsThe relevance of ambipolar diffusion for neutron star evolutionPopulation synthesis of isolated neutron stars with magneto-rotational evolution – II. From radio-pulsars to magnetarsPopulation synthesis of isolated neutron stars with magneto-rotational evoluti…A new spherically symmetric general relativistic hydrodynamical codeAnisotropic thermal emission from magnetized neutron starsEvidence for Heating of Neutron Stars by Magnetic Field DecayConstraining the GRB-magnetar model by means of the Galactic pulsar populationConstraining the GRB-magnetar model by means of the Galactic pulsar popul…The impact of magnetic field on the thermal evolution of neutron starsSpectral evolution of superluminal components in parsec-scale jetsPopulation synthesis of isolated Neutron Stars with magneto-rotational evolutionPopulation synthesis of isolated Neutron Stars with magneto-rotational evolut…Evolution of protoneutron stars with kaon condensatesNumerical relativistic hydrodynamics: Local characteristic approachPopulation synthesis studies of isolated neutron stars with magnetic field decayPopulation synthesis studies of isolated neutron stars with magnetic field dec…2D Cooling of Magnetized Neutron StarsNumerical 3+1 general relativistic magnetohydrodynamics: A Local characteristic approachNumerical 3+1 general relativistic magnetohydrodynamics: A Local characte…Magneto--thermal evolution of neutron starsNumerical {3+1} General Relativistic Hydrodynamics: A Local Characteristic ApproachNumerical {3+1} General Relativistic Hydrodynamics: A Local Characteristic …Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution modelsUnifying the observational diversity of isolated neutron stars via magneto-the…Evolution of protoneutron stars199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19901995200020052010201520202025050100150200250300350