The VLT-FLAMES Tarantula Survey - I. Introduction and observational overview
A&A, 530 (2011) A108
Published online: 2011-05-20
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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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Dynamics of young stellar clusters as planet-forming environments
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Stellar age determination in the mass–luminosity plane
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A systematic study of super-Eddington layers in the envelopes of massive stars
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A dearth of young and bright massive stars in the Small Magellanic Cloud
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Evolved massive stars at low-metallicity
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The contribution by luminous blue variable stars to the dust content of the Magellanic Clouds
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Massive stars in extremely metal-poor galaxies: a window into the past
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Supersonic turbulence in giant HII regions: clues from 30 Doradus
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The Tarantula Massive Binary Monitoring
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Physics and evolution of the most massive stars in 30 Doradus
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The B-type binaries characterization programme I. Orbital solutions for the 30 Doradus population
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Proper motions of OB stars in the far Carina Arm
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Extreme adaptive optics astrometry of R136
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Comparing hypervelocity star populations from the Large Magellanic Cloud and the Milky Way
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Mapping the core of the Tarantula Nebula with VLT-MUSE
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Detailed evolutionary models of massive contact binaries – I. Model grids and synthetic populations for the Magellanic Clouds
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VLT/X-shooter spectroscopy of massive young stellar objects in the 30 Doradus region of the Large Magellanic Cloud
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Properties of OB star−black hole systems derived from detailed binary evolution models
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Observational constraints on the likelihood of 26Al in planet-forming environments
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Core-collapse supernovae in binaries as the origin of galactic hyper-runaway stars
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Anomalous Extinction toward NGC 1938
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Atmospheric NLTE models for the spectroscopic analysis of blue stars with winds
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The R136 star cluster dissected with Hubble Space Telescope/STIS – II. Physical properties of the most massive stars in R136
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