The mass-loss dominated lives of the most massive stars
classification
🌌 astro-ph.SR
astro-ph.COastro-ph.GAastro-ph.HE
keywords
mass-losslongmassivestarsburstscalibratedominatedfates
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Utrecht has a long tradition in both spectroscopy and mass-loss studies. Here we present a novel methodology to calibrate mass-loss rates on purely spectroscopic grounds. We utilize this to predict the final fates of massive stars, involving pair-instability and long gamma-ray bursts (GRBs) at low metallicity Z.
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