Grids of stellar models with rotation VII: models from 0.8 to 300 M-circle dot at supersolar metallicity (Z=0.020)
Grids of stellar models with rotation VII: models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)
Shell model calculations of nuclear structure in "Island of inversion" N=20 region: Mg32-36 isotopes
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
Analysis of cross sections using various nuclear potential
Fate of most massive stars
Energy Loss of Neutrinos in 20Msun Star
Role of Triple Phonon Excitations on Large Angle Quasi-elastic Scattering of 54Cr+208Pb System
