Publication data of De Marco, Orsola: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2000200520102015202020250500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications20002005201020152020202502040608010003691215
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe hydrogen-deficient knot of the born again planetary nebula Abell 58 (V605 Aql)The hydrogen-deficient knot of the born again planetary nebula Abell 58 (V6…A spectroscopic analysis of blue stragglers, horizontal branch and turn-off stars in four globular clustersA spectroscopic analysis of blue stragglers, horizontal branch and turn-off sta…The Infrared L'-band view of the Galactic Center with NAOS-CONICA at VLTMid-infrared imaging of active galaxies: Active nuclei and embedded star clustersMid-infrared imaging of active galaxies: Active nuclei and embedded star clu…Adaptive optics images at 3.5 and 4.8 microns of the core arcsec of NGC 1068 : More evidence for a dusty / molecular torusAdaptive optics images at 3.5 and 4.8 microns of the core arcsec of NGC 10…V605 Aql: The Older Twin of Sakurai's ObjectBinary central stars of PN discovered through photometric variability. I. What we know and what we would like to find outBinary central stars of PN discovered through photometric variability. I. What…A new look at the evolution of wolf-rayet central stars of planetary nebulaeWolf-rayet nebulae as tracers of stellar ionizing fluxes: I. m1-67The gamma velorum binary system. 2. Wr stellar parameters and the photon loss mechanismThe gamma velorum binary system. 2. Wr stellar parameters and the photon…Accurate x-ray position of the anomalous x-ray pulsar XTE J1810-197 and identification of its likely IR counterpartAccurate x-ray position of the anomalous x-ray pulsar XTE J1810-197 and ide…Indications of a large fraction of spectroscopic binaries among nuclei of planetary nebulaeIndications of a large fraction of spectroscopic binaries among nuclei of plane…Common envelopes in massive stars: towards the role of radiation pressure and recombination energy in ejecting red supergiant envelopesCommon envelopes in massive stars: towards the role of radiation pressure a…Do most planetary nebulae derive from binaries? 1. Population synthesis model of the galactic planetary nebula population produced by singlestars and binariesDo most planetary nebulae derive from binaries? 1. Population synthesis mod…Simulations of common-envelope evolution in binary stellar systems: physical models and numerical techniquesSimulations of common-envelope evolution in binary stellar systems: physical…On the {alpha} formalism for the common envelope interactionThe Origin and Shaping of Planetary Nebulae: Putting the Binary Hypothesis to the TestThe Origin and Shaping of Planetary Nebulae: Putting the Binary Hypothesis …Simulating the Common Envelope Phase of a Red Giant Using SPH and Uniform Grid CodesSimulating the Common Envelope Phase of a Red Giant Using SPH and Unifor…Common Envelope Evolution: Where we stand and how we can move forward2000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The hydrogen-deficient knot of the born again planetary nebula Abell 58 (V605 Aql)The hydrogen-deficient knot of the born again planetary nebula Abell 58 (V6…A spectroscopic analysis of blue stragglers, horizontal branch and turn-off stars in four globular clustersA spectroscopic analysis of blue stragglers, horizontal branch and turn-off sta…The Infrared L'-band view of the Galactic Center with NAOS-CONICA at VLTMid-infrared imaging of active galaxies: Active nuclei and embedded star clustersMid-infrared imaging of active galaxies: Active nuclei and embedded star clu…Adaptive optics images at 3.5 and 4.8 microns of the core arcsec of NGC 1068 : More evidence for a dusty / molecular torusAdaptive optics images at 3.5 and 4.8 microns of the core arcsec of NGC 10…V605 Aql: The Older Twin of Sakurai's ObjectBinary central stars of PN discovered through photometric variability. I. What we know and what we would like to find outBinary central stars of PN discovered through photometric variability. I. What…A new look at the evolution of wolf-rayet central stars of planetary nebulaeWolf-rayet nebulae as tracers of stellar ionizing fluxes: I. m1-67The gamma velorum binary system. 2. Wr stellar parameters and the photon loss mechanismThe gamma velorum binary system. 2. Wr stellar parameters and the photon…Accurate x-ray position of the anomalous x-ray pulsar XTE J1810-197 and identification of its likely IR counterpartAccurate x-ray position of the anomalous x-ray pulsar XTE J1810-197 and ide…Indications of a large fraction of spectroscopic binaries among nuclei of planetary nebulaeIndications of a large fraction of spectroscopic binaries among nuclei of plane…Common envelopes in massive stars: towards the role of radiation pressure and recombination energy in ejecting red supergiant envelopesCommon envelopes in massive stars: towards the role of radiation pressure a…Do most planetary nebulae derive from binaries? 1. Population synthesis model of the galactic planetary nebula population produced by singlestars and binariesDo most planetary nebulae derive from binaries? 1. Population synthesis mod…Simulations of common-envelope evolution in binary stellar systems: physical models and numerical techniquesSimulations of common-envelope evolution in binary stellar systems: physical…On the {alpha} formalism for the common envelope interactionThe Origin and Shaping of Planetary Nebulae: Putting the Binary Hypothesis to the TestThe Origin and Shaping of Planetary Nebulae: Putting the Binary Hypothesis …Simulating the Common Envelope Phase of a Red Giant Using SPH and Uniform Grid CodesSimulating the Common Envelope Phase of a Red Giant Using SPH and Unifor…Common Envelope Evolution: Where we stand and how we can move forward2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200