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Long γ-ray bursts and core-collapse supernovae have different environmentsA debris disk around an isolated young neutron starYellow supergiants as supernova progenitors: an indication of strong mass loss for red supergiants?Gravitational Waves from Gravitational CollapseFundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before deathGravitational Waves from Gravitational Collapse.Supernovae, neutrinos and the chirality of amino acidsThe Evolution of Compact Binary Star Systems.The Evolution of Compact Binary Star Systems.Gamma-ray bursts and their use as cosmic probesAstrophysics: Going supernova.Luminous blue variables and the fates of very massive stars.Massive stars in their death throes.Cosmic ray electrons and positrons from supernova explosions of massive stars.The supernova-gamma-ray burst-jet connection.Neutrino signals from the formation of a black hole: A probe of the equation of state of dense matter.VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A),σOph, BM Sco, and HD 206859The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a {Gamma}-dependence of Wolf-Rayet type mass lossGrids of stellar models with rotationThe death of massive stars - II. Observational constraints on the progenitors of Type Ibc supernovaeThe disappearance of the progenitor of SN 2012aw in late-time imagingBinary progenitor models of type IIb supernovaeThe superluminous supernova PS1-11ap: bridging the gap between low and high redshiftCore-collapse explosions of Wolf-Rayet stars and the connection to Type IIb/Ib/Ic supernovaeThe birth of a galaxy – III. Propelling reionization with the faintest galaxiesSN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phaseLow luminosity Type II supernovae – II. Pointing towards moderate mass precursorsLocations of peculiar supernovae as a diagnostic of their originsSupernova 2012ec: identification of the progenitor and early monitoring with PESSTO★Stellar forensics with the supernova-GRB connection - Ludwig Biermann Award Lecture 2010Formation and evolution of primordial protostellar systemsTesting the predicted mass-loss bi-stability jump at radio wavelengthsPair creation supernovae at low and high redshiftProduction of dust by massive stars at high redshiftGenesis and evolution of dust in galaxies in the early UniverseNew signature of dark matter annihilations: Gamma rays from intermediate-mass black holesBinary companions of nearby supernova remnants found with GaiaSearch for gravitational waves associated with the gamma ray burst GRB030329 using the LIGO detectorsOptical photometry and spectroscopy of the low-luminosity, broad-lined Ic supernova iPTF15dldThe MUSE view of the host galaxy of GRB 100316D
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P2860
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Juli 2003 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в липні 2003
@uk
name
How Massive Single Stars End Their Life
@en
How Massive Single Stars End Their Life
@nl
type
label
How Massive Single Stars End Their Life
@en
How Massive Single Stars End Their Life
@nl
prefLabel
How Massive Single Stars End Their Life
@en
How Massive Single Stars End Their Life
@nl
P2093
P356
P1476
How Massive Single Stars End Their Life
@en
P2093
C. L. Fryer
D. H. Hartmann
S. E. Woosley
P304
P356
10.1086/375341
P407
P577
2003-07-01T00:00:00Z
P5875
P818
astro-ph/0212469
P819
2003ApJ...591..288H