On the metallicity dependence of Wolf-Rayet winds
A&A, 442 2 (2005) 587-596
Published online: 2005-10-07
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Why Are Some Gamma-Ray Bursts Hosted by Oxygen-rich Galaxies?
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Subsonic structure and optically thick winds from Wolf–Rayet stars
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Investigating a population of infrared-bright gamma-ray burst host galaxies
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How common is LBV S Doradus variability at low metallicity?
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Helium Star Models with Optically Thick Winds: Implications for the Internal Structures and Mass-loss Rates of Wolf–Rayet Stars
Daisuke Nakauchi and Hideyuki SaioThe Astrophysical Journal 852 (2) 126 (2018)
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The environment of the SN-less GRB 111005A at z = 0.0133
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Related Progenitor Models for Long-duration Gamma-Ray Bursts and Type Ic Superluminous Supernovae
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Accuracy of inference on the physics of binary evolution from gravitational-wave observations
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Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
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Black hole demography at the dawn of gravitational-wave astronomy: state-of-the art and future perspectives
Michela MapelliJournal of Physics: Conference Series 957 012001 (2018)
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ZFIRE: using Hα equivalent widths to investigate the in situ initial mass function at z ∼ 2
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Formation of the first three gravitational-wave observations through isolated binary evolution
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Revealing Black Holes with Gaia
Katelyn Breivik, Sourav Chatterjee and Shane L. LarsonThe Astrophysical Journal Letters 850 (1) L13 (2017)
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Ultraviolet spectra of extreme nearby star-forming regions – approaching a local reference sample for JWST
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