The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
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The VLT-FLAMES Tarantula SurveyGamma-ray burst progenitors and the population of rotating Wolf-Rayet stars.The Evolution of Compact Binary Star Systems.Mass loss and stellar superwinds.How does a low-mass cut-off in the stellar IMF affect the evolution of young star clusters?The discovery of a very massive star in W49The evolution of massive stars and their spectra. I. A non-rotating 60 M_{sun}_ star from the zero-age main sequence to the pre-supernova stageThe VLT-FLAMES Tarantula SurveyThe Wolf-Rayet stars in the Large Magellanic CloudThe R136 star cluster dissected withHubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He ii λ1640 in young star clustersThe Eddington factor as the key to understand the winds of the most massive stars. Evidence for a {Gamma}-dependence of Wolf-Rayet type mass lossGrids of stellar models with rotationTwo massive stars possibly ejected from NGC 3603 via a three-body encounterThe VLT-FLAMES Tarantula SurveyThe emergence of super-canonical stars in R136-type starburst clustersSpectral classification of O2-3.5 If*/WN5-7 starsEvolution and fate of very massive starsCore-collapse explosions of Wolf-Rayet stars and the connection to Type IIb/Ib/Ic supernovaeA Galactic O2 If*/WN6 star possibly ejected from its birthplace in NGC 3603The evolution of rotating very massive stars with LMC compositionVery Massive Stars in the local UniverseSteady outflows in giant clumps of high-z disc galaxies during migration and growth by accretionThe 155-day X-ray cycle of the very massive Wolf–Rayet star Melnick 34 in the Large Magellanic CloudFast evolving pair-instability supernova models: evolution, explosion, light curvesAn extremely bright gamma-ray pulsar in the Large Magellanic CloudA comprehensive comparative test of seven widely used spectral synthesis models against multi-band photometry of young massive-star clustersThe Software Package for Astronomical Reductions with KMOS: SPARKSystematic survey of the effects of wind mass loss algorithms on the evolution of single massive starsThe Tarantula Massive Binary MonitoringLow-metallicity massive single stars with rotationOn the possibility that the most massive stars result from binary mergersThe VLT-FLAMES Tarantula surveyThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyThe Tarantula Nebula as a template for extragalactic star forming regions from VLT/MUSE and HST/STISChemistry and kinematics of red supergiant stars in the young massive cluster NGC 2100Binary-corrected velocity dispersions from single- and multi-epoch radial velocities: massive stars in R136 as a test caseStudying the kinematics of the giant star-forming region 30 DoradusThe mass of the very massive binary WR21a
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P2860
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit
description
2010 nî lūn-bûn
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2010年の論文
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2010年学术文章
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2010年学术文章
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2010年学术文章
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name
The R136 star cluster hosts se ...... pted 150 M⊙ stellar mass limit
@en
The R136 star cluster hosts se ...... pted 150 M⊙ stellar mass limit
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type
label
The R136 star cluster hosts se ...... pted 150 M⊙ stellar mass limit
@en
The R136 star cluster hosts se ...... pted 150 M⊙ stellar mass limit
@nl
prefLabel
The R136 star cluster hosts se ...... pted 150 M⊙ stellar mass limit
@en
The R136 star cluster hosts se ...... pted 150 M⊙ stellar mass limit
@nl
P2093
P1476
The R136 star cluster hosts se ...... pted 150 M⊙ stellar mass limit
@en
P2093
Hasan Abu Kassim
Olivier Schnurr
Paul A. Crowther
Raphael Hirschi
Richard J. Parker
Simon P. Goodwin
P304
P356
10.1111/J.1365-2966.2010.17167.X
P407
P577
2010-07-26T00:00:00Z
P5875
P818
P819
2010MNRAS.408..731C