about
Asteroseismology can reveal strong internal magnetic fields in red giant stars.A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars.Discovery of the massive overcontact binary VFTS352: evidence for enhanced internal mixingEjection of the Massive Hydrogen-rich Envelope Timed with the Collapse of the Stripped SN 2014C.The Cepheid mass discrepancy and pulsation-driven mass lossThe VLT-FLAMES Tarantula survey: the fastest rotating o-type star and shortest period LMC Pulsar--Remnants of a supernova disrupted binary?Rotating massive main-sequence starsPair creation supernovae at low and high redshiftInference of Stellar Parameters from Brightness VariationsThe O stars in the VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula surveyRotating massive main-sequence starsThe VLT-FLAMES Tarantula SurveyChemically Homogeneous Evolution in Massive BinariesLight elements in massive single and binary starsThe VLT–FLAMES Tarantula SurveyRotational mixing in massive binaries. Detached short-period systemsRotational mixing in close binariesRotation and Massive Close Binary EvolutionThe VLT-FLAMES Tarantula SurveyUltra-long Gamma-Ray Bursts from the Collapse of Blue Supergiant Stars: An End-to-end SimulationPlanetary Engulfment in the Hertzsprung–Russell DiagramOff-axis Prompt X-Ray Transients from the Cocoon of Short Gamma-Ray BurstsThe Effects of Magnetic Fields on the Dynamics of Radiation Pressure–dominated Massive Star EnvelopesConversion of internal gravity waves into magnetic wavesSPIRITS: Uncovering Unusual Infrared Transients with SpitzerOn variations of pre-supernova model propertiesAsteroseismic signatures of evolving internal stellar magnetic fieldsMesa isochrones and stellar tracks (MIST). I solar-scaled modelsLimits on the spin up of stellar-mass black holes through a spiral stationary accretion shock instabilityERRATUM: “MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS” (2015, ApJS, 220, 15)Suppression of Quadrupole and Octupole Modes in Red Giants Observed by KeplerERRATUM: “THE SPIN RATE OF PRE-COLLAPSE STELLAR CORES: WAVE-DRIVEN ANGULAR MOMENTUM TRANSPORT IN MASSIVE STARS” (2015, ApJ, 810, 101)Local radiation hydrodynamic simulations of massive star envelopes at the iron opacity peakModules for experiments in stellar astrophysics (MESA): binaries, pulsations, and explosionsThe spin rate of pre-collapse stellar cores: wave-driven angular momentum transport in massive starsAngular momentum transport via internal gravity waves in evolving starsThe formation and gravitational-wave detection of massive stellar black hole binariesAngular momentum transport within evolved low-mass starsThe fate of fallback matter around newly born compact objects
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P50
description
hulumtues
@sq
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
M. Cantiello
@nl
M. Cantiello
@sl
Matteo Cantiello
@en
Matteo Cantiello
@es
type
label
M. Cantiello
@nl
M. Cantiello
@sl
Matteo Cantiello
@en
Matteo Cantiello
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M. Cantiello
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prefLabel
M. Cantiello
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M. Cantiello
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Matteo Cantiello
@en
Matteo Cantiello
@es
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P106
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0000-0002-8171-8596