Hello guys. I'm working to compute de max. mass for a white dwarf through solving the hidrostatic equilibrium equations. ( The classical ones, not TOV), and using an EoS made by my own, that considers the Fermi Pressure and stuff. When i use the EoS for a carbon white dwarf ( i do get the Chandrasekhar mass correctly, but if i use for Iron i get i bit less then it should be. ( 1,23 instead 1,46 solar masses) So. This difference really exist or i'm getting it wrong ??