Dark energy stars in the context of black holes - The physical profiles
Grids of stellar models with rotation VII: models from 0.8 to 300 M-circle dot at supersolar metallicity (Z=0.020)
Very massive star winds as sources of the short-lived radioactive isotope Al-26
The neutrino emission from thermal processes in very massive stars in the local universe
Evolution of solar-like stars. HA Kassim, N Yusof, M Idris and ZA Motahar
Stellar Models with Rotation at High Metallicitiy
Energy Loss of Neutrinos in 20 Msun and 40 Msun Massive Stars
Solar Neutrino Fluxes Using The Exponential S-Factor
The Exponential S-Factor in the PP Chain
