Publication data of Christodoulou, Dimitris M.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250100200300400500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250122436486001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025024681012
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestDominance of outflowing electric currents on decaparsec to kiloparsec scales in extragalactic jetsDominance of outflowing electric currents on decaparsec to kiloparsec scales…The X-ray Binary Population of the Nearby Dwarf Starburst Galaxy IC 10: Variable and Transient X-ray SourcesThe X-ray Binary Population of the Nearby Dwarf Starburst Galaxy IC 10: Vari…Not an oxymoron: some X-ray binary pulsars with enormous spin-up rates reveal weak magnetic fieldsNot an oxymoron: some X-ray binary pulsars with enormous spin-up rates rev…The stability of accretion tori. 5. Unstable modes and avoided crossings in extended, selfgravitating annuliThe stability of accretion tori. 5. Unstable modes and avoided crossings in ex…Interchange method in compressible magnetized Couette flow: Magnetorotational and magnetoconvective instabilitiesInterchange method in compressible magnetized Couette flow: Magnetorotat…The X-ray Pulsar M82 X-2 on its Propeller LineRetrograde accretion discs in high-mass Be/X-ray binariesInterposing a Varying Gravitational Constant Between Modified Newtonian Dynamics and Weak Weyl GravityInterposing a Varying Gravitational Constant Between Modified Newtonian Dy…Determination of the Magnetic Fields of Magellanic X-Ray PulsarsInfrared search for young stars in hi high-velocity cloudsA new criterion for bar-forming instability in rapidly rotating gaseous and stellar systems. 2. Nonaxisymmetric formA new criterion for bar-forming instability in rapidly rotating gaseous and stell…Phase-Transition Theory of Instabilities.I.Second-Harmonic Instability and Bifurcation PointsPhase-Transition Theory of Instabilities.I.Second-Harmonic Instability and Bifu…Simulations of the Poynting-Robertson Cosmic Battery in Resistive Accretion DisksSimulations of the Poynting-Robertson Cosmic Battery in Resistive Accretion …The Wolf-Rayet + Black Hole Binary NGC 300 X-1: What is the Mass of the Black Hole?The Wolf-Rayet + Black Hole Binary NGC 300 X-1: What is the Mass of the Bla…The Cosmic Battery RevisitedThe invariant Twist of Magnetic Fields in the Relativistic Jets of Active Galactic NucleiThe invariant Twist of Magnetic Fields in the Relativistic Jets of Active Galactic …A Comprehensive Library of X-ray Pulsars in the Small Magellanic Cloud: Time Evolution of their Luminosities and Spin PeriodsA Comprehensive Library of X-ray Pulsars in the Small Magellanic Cloud: Time…Revisiting the Dynamical Case for a Massive Black Hole in IC10 X-1A new criterion for bar-forming instability in rapidly rotating gaseous and stellar systems. I. axisymmetric formA new criterion for bar-forming instability in rapidly rotating gaseous and stell…19952000200520102015202020250100200300400500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Dominance of outflowing electric currents on decaparsec to kiloparsec scales in extragalactic jetsDominance of outflowing electric currents on decaparsec to kiloparsec scales…The X-ray Binary Population of the Nearby Dwarf Starburst Galaxy IC 10: Variable and Transient X-ray SourcesThe X-ray Binary Population of the Nearby Dwarf Starburst Galaxy IC 10: Vari…Not an oxymoron: some X-ray binary pulsars with enormous spin-up rates reveal weak magnetic fieldsNot an oxymoron: some X-ray binary pulsars with enormous spin-up rates rev…The stability of accretion tori. 5. Unstable modes and avoided crossings in extended, selfgravitating annuliThe stability of accretion tori. 5. Unstable modes and avoided crossings in ex…Interchange method in compressible magnetized Couette flow: Magnetorotational and magnetoconvective instabilitiesInterchange method in compressible magnetized Couette flow: Magnetorotat…The X-ray Pulsar M82 X-2 on its Propeller LineRetrograde accretion discs in high-mass Be/X-ray binariesInterposing a Varying Gravitational Constant Between Modified Newtonian Dynamics and Weak Weyl GravityInterposing a Varying Gravitational Constant Between Modified Newtonian Dy…Determination of the Magnetic Fields of Magellanic X-Ray PulsarsInfrared search for young stars in hi high-velocity cloudsA new criterion for bar-forming instability in rapidly rotating gaseous and stellar systems. 2. Nonaxisymmetric formA new criterion for bar-forming instability in rapidly rotating gaseous and stell…Phase-Transition Theory of Instabilities.I.Second-Harmonic Instability and Bifurcation PointsPhase-Transition Theory of Instabilities.I.Second-Harmonic Instability and Bifu…Simulations of the Poynting-Robertson Cosmic Battery in Resistive Accretion DisksSimulations of the Poynting-Robertson Cosmic Battery in Resistive Accretion …The Wolf-Rayet + Black Hole Binary NGC 300 X-1: What is the Mass of the Black Hole?The Wolf-Rayet + Black Hole Binary NGC 300 X-1: What is the Mass of the Bla…The Cosmic Battery RevisitedThe invariant Twist of Magnetic Fields in the Relativistic Jets of Active Galactic NucleiThe invariant Twist of Magnetic Fields in the Relativistic Jets of Active Galactic …A Comprehensive Library of X-ray Pulsars in the Small Magellanic Cloud: Time Evolution of their Luminosities and Spin PeriodsA Comprehensive Library of X-ray Pulsars in the Small Magellanic Cloud: Time…Revisiting the Dynamical Case for a Massive Black Hole in IC10 X-1A new criterion for bar-forming instability in rapidly rotating gaseous and stellar systems. I. axisymmetric formA new criterion for bar-forming instability in rapidly rotating gaseous and stell…19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250102030405060