Stellar Properties of Observed Stars Stripped in Binaries in the Magellanic Clouds

Keyphrases

• Atmosphere Model 33%
• Binary Evolution 66%
• Binary Interaction 33%
• Bolometric Luminosity 33%
• Computing Model 33%
• Core-collapse 33%
• Eddington 33%
• Effective Temperature 33%
• Emission Rate 33%
• Evolution Model 33%
• Helium 100%
• Hydrogen-rich 33%
• Intermediate Mass 33%
• Magellanic Clouds 100%
• Mass Loss Rate 33%
• Massive Stars 66%
• Model Fitting 33%
• Neutron Stars 66%
• Population Synthesis 33%
• Small Radius 33%
• Stellar Properties 100%
• Stellar Winds 33%
• Supernovae 66%
• Surface Gravity 33%
• Surfing 33%
• Synthesis Model 33%

Physics

• B Stars 50%
• Black Holes 50%
• Magellanic Clouds 100%
• Massive Star 100%
• Neutron Stars 100%
• Planetary Atmosphere 50%
• Stellar Wind 50%
• Supernovae 100%
• Surface Gravity 50%