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Dynamical age differences among coeval star clusters as revealed by blue stragglers.The radial distribution of blue straggler stars and the nature of their progenitorsNGC 2276: a remarkable galaxy with a large number of ultraluminous X-ray sourcesThe population of ULXs in the spiral galaxy NGC 2276C7 multi-messenger astronomy of GW sourcesEccentric disc instability in stellar discs formed from inspiralling gas clouds in the Galactic CentrePeriodic signals from the Circinus region: two new cataclysmic variables and the ultraluminous X-ray source candidate GC X-1Swift J201424.9+152930: discovery of a new deeply eclipsing binary with 491-s and 3.4-h modulationsDiscovery of a 6.4 h black hole binary in NGC 4490Constraints on Galactic intermediate mass black holesGASP V: Ram-pressure stripping of a ring Hoag’s-like galaxy in a massive clusterTheGaia-ESO survey: Discovery of a spatially extended low-mass population in the Vela OB2 associationUltraluminous X-ray Sources forming in low metallicity natal environmentsImpact of dark matter decays and annihilations on reionizationThe ACS LCID project. VII. The blue stragglers population in the isolated dSph galaxies Cetus and TucanaBlue straggler stars in dwarf spheroidal galaxies - II. Sculptor and FornaxA Panchromatic Study of the Globular Cluster NGC 1904. I. The Blue Straggler PopulationBlue straggler stars in dwarf spheroidal galaxiesThe Blue Straggler Population of the Globular Cluster M5The fingerprint of binary intermediate-mass black holes in globular clusters: suprathermal stars and angular momentum alignmentThe Contribution of Primordial Binaries to the Blue Straggler Population in 47 TucanaeUltra-luminous X-ray sources and remnants of massive metal-poor starsRoche-lobe overflow systems powered by black holes in young star clusters: the importance of dynamical exchangesA disrupted bulgeless satellite galaxy as counterpart of the ultraluminous X-ray source ESO 243-49 HLX-1A minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1 – II. Constraints from photometryDynamics of stellar black holes in young star clusters with different metallicities – I. Implications for X-ray binariesA minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1Dynamics of massive stellar black holes in young star clusters and the displacement of ultra-luminous X-ray sourcesRemnants of massive metal-poor stars: Viable engines for ultra-luminous X-ray sourcesThe metallicity of the nebula surrounding the ultra-luminous X-ray source NGC 1313 X-2Low metallicity and ultra-luminous X-ray sources in the Cartwheel galaxyLopsided galaxies: the case of NGC 891Evolution of dwarf galaxies hosting GW150914-like eventsThe formation and coalescence sites of the first gravitational wave eventsGamma-ray constraints on the infrared background excessSearch for Subsolar Mass Ultracompact Binaries in Advanced LIGO's Second Observing RunBlack-Hole Remnants from Black-Hole-Neutron-Star Mergers
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description
researcher ORCID ID = 0000-0001-8799-2548
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wetenschapper
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name
M Mapelli
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M Mapelli
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M Mapelli
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M Mapelli
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type
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M Mapelli
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M Mapelli
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M Mapelli
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M Mapelli
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prefLabel
M Mapelli
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M Mapelli
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M Mapelli
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M Mapelli
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P106
P1153
55941312500
P31
P496
0000-0001-8799-2548