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Physical Properties of Wolf-Rayet Stars

Annual review of astronomy and astrophysics, 2007-01, Vol.45 (1), p.177-219

Crowther, Paul A

2007

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The luminosities of cool supergiants in the Magellanic Clouds, and the Humphreys–Davidson limit revisited

Monthly notices of the Royal Astronomical Society, 2018-08, Vol.478 (3), p.3138-3148

2018

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Massive Stars in the Tarantula Nebula: A Rosetta Stone for Extragalactic Supergiant HII Regions

Galaxies, 2019-12, Vol.7 (4), p.88

Crowther, Paul A.

2019

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On the association between core-collapse supernovae and H ii regions

Monthly notices of the Royal Astronomical Society, 2013-01, Vol.428 (3), p.1927-1943

Crowther, Paul A.

2013

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The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources

The Astrophysical journal, 2022-01, Vol.925 (1), p.69

2022

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Origins of Type Ibn SNe 2006jc/2015G in interacting binaries and implications for pre-SN eruptions

Monthly notices of the Royal Astronomical Society, 2020-02, Vol.491 (4), p.6000-6019

2020

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The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit

Monthly notices of the Royal Astronomical Society, 2010-10, Vol.408 (2), p.731-751

2010

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Spectral classification of O2-3.5 If/WN5-7 stars

Monthly notices of the Royal Astronomical Society, 2011-09, Vol.416 (2), p.1311-1323

2011

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Chemical Abundances in the Leading Arm of the Magellanic Stream

The Astrophysical journal, 2018-02, Vol.854 (2), p.142

2018

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Unlocking Galactic Wolf–Rayet stars with Gaia DR2 – I. Distances and absolute magnitudes

Monthly notices of the Royal Astronomical Society, 2020-03, Vol.493 (1), p.1512-1529

2020

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Mapping the core of the Tarantula Nebula with VLT-MUSE – III. A template for metal-poor starburst regions in the visual and far-ultraviolet

Monthly notices of the Royal Astronomical Society, 2024-01, Vol.527 (3), p.9023-9047

2024

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The G305 star-forming complex: the central star clusters Danks 1 and Danks 2

Monthly notices of the Royal Astronomical Society, 2012-01, Vol.419 (3), p.1871-1886

2012

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Unlocking Galactic Wolf–Rayet stars with Gaia DR2 – II. Cluster and association membership

Monthly notices of the Royal Astronomical Society, 2020-06, Vol.495 (1), p.1209-1226

2020

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Line luminosities of Galactic and Magellanic Cloud Wolf–Rayet stars

Monthly notices of the Royal Astronomical Society, 2023-05, Vol.521 (1), p.585-612

2023

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Evolution and fate of very massive stars

Monthly notices of the Royal Astronomical Society, 2013-08, Vol.433 (2), p.1114-1132

2013

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The changing-type SN 2014C may come from an 11-M⊙ star stripped by binary interaction and violent eruption

Monthly notices of the Royal Astronomical Society, 2020-10, Vol.497 (4), p.5118-5135

2020

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A UV census of the environments of stripped-envelope supernovae

Monthly notices of the Royal Astronomical Society, 2023-05, Vol.521 (2), p.2860-2873

2023

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Spectral classification of O2-3.5If/WN5-7 stars

Monthly notices of the Royal Astronomical Society, 2011-09, Vol.416 (2), p.1311-1323

2011

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A hot and luminous source at the site of the fast transient AT2018cow at 2–3 yr after its explosion

Monthly notices of the Royal Astronomical Society. Letters, 2022-05, Vol.512 (1), p.L66-L70

2022

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MSX mid-infrared imaging of massive star birth environments - II. Giant H ii regions

Monthly notices of the Royal Astronomical Society, 2004-12, Vol.355 (3), p.899-917

2004

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The R136 star cluster dissected with Hubble Space Telescope/STIS – II. Physical properties of the most massive stars in R136

Monthly notices of the Royal Astronomical Society, 2020-12, Vol.499 (2), p.1918-1936

2020

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An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion

Monthly notices of the Royal Astronomical Society, 2022-03, Vol.510 (3), p.3701-3715

2022

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Grids of stellar models with rotation VII: models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)

Monthly notices of the Royal Astronomical Society, 2022-04, Vol.511 (2), p.2814-2828

2022

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ULLYSES and Complementary Surveys of Massive Stars in the Magellanic Clouds

Proceedings of the International Astronomical Union, 2022-05, Vol.18 (S361), p.15-25

Crowther, Paul A.

2022

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Towards a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE

Monthly notices of the Royal Astronomical Society, 2021-06, Vol.504 (2), p.2253-2272

2021

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Physical Properties of Wolf-Rayet Stars

The luminosities of cool supergiants in the Magellanic Clouds, and the Humphreys–Davidson limit revisited

Massive Stars in the Tarantula Nebula: A Rosetta Stone for Extragalactic Supergiant HII Regions

On the association between core-collapse supernovae and H ii regions

The Uncertain Future of Massive Binaries Obscures the Origin of LIGO/Virgo Sources

Origins of Type Ibn SNe 2006jc/2015G in interacting binaries and implications for pre-SN eruptions

The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit

Spectral classification of O2-3.5 If/WN5-7 stars

Chemical Abundances in the Leading Arm of the Magellanic Stream

Unlocking Galactic Wolf–Rayet stars with Gaia DR2 – I. Distances and absolute magnitudes

Mapping the core of the Tarantula Nebula with VLT-MUSE – III. A template for metal-poor starburst regions in the visual and far-ultraviolet

The G305 star-forming complex: the central star clusters Danks 1 and Danks 2

Unlocking Galactic Wolf–Rayet stars with Gaia DR2 – II. Cluster and association membership

Line luminosities of Galactic and Magellanic Cloud Wolf–Rayet stars

Evolution and fate of very massive stars

The changing-type SN 2014C may come from an 11-M⊙ star stripped by binary interaction and violent eruption

A UV census of the environments of stripped-envelope supernovae

Spectral classification of O2-3.5If/WN5-7 stars

A hot and luminous source at the site of the fast transient AT2018cow at 2–3 yr after its explosion

MSX mid-infrared imaging of massive star birth environments - II. Giant H ii regions

The R136 star cluster dissected with Hubble Space Telescope/STIS – II. Physical properties of the most massive stars in R136

An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion

Grids of stellar models with rotation VII: models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)

ULLYSES and Complementary Surveys of Massive Stars in the Magellanic Clouds

Towards a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE

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