Very massive star winds as sources of the short-lived radioactive isotope Al-26
Grids of stellar models with rotation VII: models from 0.8 to 300 M-circle dot at supersolar metallicity (Z=0.020)
The neutrino emission from thermal processes in very massive stars in the local universe
Grids of stellar models with rotation VI. Models from 0.8 to 120 M-circle dot at a metallicity Z=0.006
Evolution of solar-like stars. HA Kassim, N Yusof, M Idris and ZA Motahar
Very Massive Stars and the Eddington Limit
Fate of most massive stars
Solar Modeling with MESA Code
Energy Loss of Neutrinos in 20 Msun and 40 Msun Massive Stars
