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R145
R136: the Core of the Lonizing Cluster of 30 Doradus J
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS
R144 Revealed As a Double-Lined Spectroscopic Binary?
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
The VLT-FLAMES Tarantula Survey ⋆⋆⋆⋆⋆⋆
Refereed Publications Selma E De Mink Generated Automatically from NASA ADS Database on 8Th August 2019
The Tarantula Massive Binary Monitoring Project: II. a First SB2
A Wind-Eclipsing Binary with a Total Mass 140 M
Dr. S. (Selma) E. De Mink Astrophysicist - Macgillavry Assistant Professor Anton Pannekoek Instituut Voor Sterrenkunde, Univ
Massive Stars - Binaries, Wolf-Rayets, and the Early Universe Connection
Atmospheric Photochemistry, Surface Features, and Potential Biosignature Gases of Terrestrial Exoplanets by Renyu Hu M.S
Arxiv:Astro-Ph/0106109V2 9 Apr 2002
THE MAGELLANIC CLOUDS NEWSLETTER an Electronic Publication Dedicated to the Magellanic Clouds, and Astrophysical Phenomena Therein
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS
Multiplicity of Massive Stars
The VLT-FLAMES Tarantula Survey XI. a Census of the Hot Luminous Stars and Their Feedback in 30 Doradus
The Evolution of Massive Stars in the Small Magellanic Cloud
The VLT-FLAMES Tarantula Survey
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The Multiplicity of Massive Stars: a 2016 View
Massive Stars in the Tarantula Nebula: a Rosetta Stone for Extragalactic Supergiant HII Regions
II. First SB2 Orbital and Spectroscopic Analysis for the Wolf-Rayet Binary R145?
On the Origin of the Most Massive Stars Around R136
Manual on Air Traffic Management System Requirements
The R136 Star Cluster Dissected with Hubble Space Telescope/STIS. I
A Chandra/ACIS Study of 30 Doradus II. X-Ray Point Sources in The
The Ultraviolet Extinction Properties of the Tarantula Nebula
Properties of Extragalactic Wolf-Rayet Stars
Redalyc.A GLOBAL ASSESSMENT of WOLF-RAYET BINARIES IN
Annual Energy Review 2011
He II M686 in TJ CARINAE: COLLAPSE of the WIND-WIND COLLISION REGION DURING PERIASTRON PASSAGE U