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)
Grids of stellar models with rotation VII: models from 0.8 to 300 M⊙ at supersolar metallicity (Z = 0.020)
The Effect of the Quantization of the Centrifugal Stretching on the Analysis of the Rotational Spectra of Even-Even Nuclei
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
