15 solar masses model s15

• Solar neutrinos and geoneutrinos versus pre-supernova @ 1 kiloparsec. 40,000 years before core-collapse supernova [AVI]
  
  
• Surface versus central evolution [AVI]
  
  
• Electron anti-neutrino emissivity [erg/cc] [AVI]
  
  
• Mean energy of the electron anti-neutrinos [AVI]
  
  
• Combined mean energy and emissivity of the electron anti-neutrinos [AVI]
  
  
• Electron anti-neutrino emissivity [erg/g] [AVI]