Paul Crowther
1934
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country of citizenship: United Kingdom
languages spoken, written or signed: English
educated at: University College London
occupation: researcher
Works 1
Articles 196
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An X-ray-quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud
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The Tarantula Massive Binary Monitoring
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Two Wolf-Rayet stars at the heart of colliding-wind binary Apep
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The extreme colliding-wind system Apep: resolved imagery of the central binary and dust plume in the infrared
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The 3D shape of Type IIb SN 2011hs
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Investigating the origin of the spectral line profiles of the Hot Wolf–Rayet Star WR 2
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Weighing Melnick 34: the most massive binary system known
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Anisotropic winds in a Wolf-Rayet binary identify a potential gamma-ray burst progenitor
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An excess of massive stars in the local 30 Doradus starburst.
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Probing the rotational velocity of Galactic WO stars with spectropolarimetry
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Response to Comment on “An excess of massive stars in the local 30 Doradus starburst”
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Spectral models for binary products: Unifying subdwarfs and Wolf-Rayet stars as a sequence of stripped-envelope stars
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HST Astrometry in the 30 Doradus Region. II. Runaway Stars from New Proper Motions in the Large Magellanic Cloud
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Investigating the properties of stripped-envelope supernovae; what are the implications for their progenitors?
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Gaia DR2 reveals a very massive runaway star ejected from R136
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The first optical spectra of Wolf-Rayet stars in M101 revealed with Gemini/GMOS
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The VLT-FLAMES Tarantula Survey. XXVIII. Nitrogen abundances for apparently single dwarf and giant B-type stars with small projected rotational velocities
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Mapping the core of the Tarantula Nebula with VLT-MUSE. I. Spectral and nebular content around R136
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The luminosities of cool supergiants in the Magellanic Clouds, and the Humphreys-Davidson limit revisited
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The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst
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Chemical Abundances in the Leading Arm of the Magellanic Stream
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Anisotropic winds in a Wolf–Rayet binary identify a potential gamma-ray burst progenitor
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Bridging the gap: from massive stars to supernovae
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The 155-day X-ray cycle of the very massive Wolf–Rayet star Melnick 34 in the Large Magellanic Cloud
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The VLT-FLAMES Tarantula Survey. XXVII. Physical parameters of B-type main-sequence binary systems in the Tarantula nebula
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The VLT-FLAMES Tarantula Survey. XXVI. Properties of the O-dwarf population in 30 Doradus
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The VLT-FLAMES Tarantula Survey. XXV. Surface nitrogen abundances of O-type giants and supergiants
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The Tarantula Massive Binary Monitoring
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The Tarantula Massive Binary Monitoring
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The VLT-FLAMES Tarantula Survey
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Revealing the nebular properties and Wolf-Rayet population of IC10 with Gemini/GMOS
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Gamma-Ray Burst Progenitors
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