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R136
The Central Density of R136 in 30 Doradus
Curriculum Vitae of You-Hua Chu
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS. II
R136: the Core of the Lonizing Cluster of 30 Doradus J
HST SCIENCE and DISCOVERIES T
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS
Dissecting the Core of the Tarantula Nebula with MUSE
Super Star Cluster R136: Puzzles Outside and Inside
REFEREED PUBLICATIONS of YOU-HUA CHU A. Articles in Journals
The Most Massive LMC Star Sk-66°41 Resolved
The VLT FLAMES Tarantula Survey
A Complete Massive Star Census of R136/NGC2070: the Core of 30
The Star-Forming Complex LMC-N79 As a Future Rival to 30 Doradus
Very Massive Stars in Super Star Clusters
Arxiv:1702.03108V1 [Astro-Ph.GA] 10 Feb 2017 Results from Nearby, Resolved Star-Forming Regions
Arxiv:1711.03153V2 [Astro-Ph.GA] 10 Nov 2017 10 M Within 10 Pc (Selman & Melnick 2013)
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS
R144: a Very Massive Binary Likely Ejected from R136 Through a Binary–Binary Encounter
Top View
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
Commission 45: Stellar Classification (Classification Stellaire)
Hot Massive Stars: the Impact Of
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
© American Astronomical Society • Provided by the NASA Astrophysics
Structure and Feedback in 30 Doradus. Ii. Structure and Chemical Abundances
The Ultraviolet Extinction Properties of the Tarantula Nebula
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS. II
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS
Extreme Adaptive Optics Astrometry of R136 Searching for High Proper Motion Stars?,??
The Initial Mass Function and Star Formation Law in the Outer Disc of NGC 2915
13052 (Stsci Edit Number: 2, Created: Friday, July 6, 2012 9:21:02 PM EST) - Overview
Dissecting the Core of the Tarantula Nebula with MUSE
VFTS 682, an Isolated ~130 MΘ Twin of R136's Wn5h Core Stars