Extreme isolation of WN3/O3 stars and implications for their evolutionary origin as the elusive stripped binaries

Keyphrases

• Massive Stars 100%
• Evolutionary Origin 100%
• Stripped Binaries 100%
• Low-mass 66%
• Initial Mass 66%
• Wolf-Rayet Stars 66%
• O-type 66%
• Radial Velocity 33%
• Luminosity 33%
• Supernovae 33%
• Red Supergiants 33%
• Mass Range 33%
• Spatial Distribution 33%
• Luminous Blue Variables 33%
• Runaway 33%
• Magellanic Clouds 33%
• Large Magellanic Cloud 33%
• Interacting Binaries 33%
• High-resolution Spectra 33%
• Hertzsprung-Russell Diagram 33%
• Wolf-Rayet 33%
• Binary Model 33%
• Non-conservative Mass Transfer 33%

Physics

• Massive Star 100%
• Wolf-Rayet Star 66%
• Supernovae 33%
• Red Supergiant Stars 33%
• High Resolution 33%
• Radial-Velocity Method 33%
• Luminous Blue Variable Stars 33%
• Large Magellanic Cloud 33%
• Magellanic Clouds 33%
• Spatial Distribution 33%
• Hertzsprung-Russell Diagram 33%
• WN Stars 33%