R136
![Arxiv:1702.03108V1 [Astro-Ph.GA] 10 Feb 2017 Results from Nearby, Resolved Star-Forming Regions](http://data.docslib.org/img/264x/527798932010470a75b530902dc4ae9b.webp)
![Arxiv:1711.03153V2 [Astro-Ph.GA] 10 Nov 2017 10 M Within 10 Pc (Selman & Melnick 2013)](http://data.docslib.org/img/264x/52f61666d898e97fd758e94db9540916.webp)
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- The R136 Star Cluster Hosts Several Stars Whose Individual Masses Greatly Exceed the Accepted 150 M⊙ Stellar Mass Limit
- Hénault-Brunet Et
- The Very Massive and Hot LMC Star VFTS 682: Progenitor of a Future Dark Gamma-Ray Burst?
- X-Rays from Superbubbles in the Large Magellanic Cloud. V. the H II
- Download This Article in PDF Format
- Formation and Evolution of Massive Stars: Current Surveys
- Paul Crowther (University of Sheffield) Science with the HST IV: Looking to the Future Outline
- The Origin of OB Runaway Stars by the Supernova Explosion of a Stellar Companion (3)
- The Role of Stellar Feedback in the Dynamics of H Ii Regions
- Towards a Sharper Picture of R136 with SPHERE Extreme Adaptive Optics
- 15942 (Stsci Edit Number: 0, Created: Thursday, March 5, 2020 at 12:00:37 PM Eastern Standard Time) - Overview
- Massive Stars in the Tarantula Nebula: a Rosetta Stone for Extragalactic Supergiant HII Regions
- Star Formation and Feedback in the SOFIA Era Celebrating 50 Years of Airborne Astronomy
- THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
- Press Release
- The 155-Day X-Ray Cycle of the Very Massive Wolf-Rayet Star Melnick 34 in the Large Magellanic Cloud
- The VLT-FLAMES Tarantula Survey III: a Very Massive Star in Apparent Isolation from the Massive Cluster R136? Joachim M
- On the Origin of the Most Massive Stars Around R136