4.3) and because (2) models in this mass range are expected to become core-hydrogen-burning SG stars (cf. Sect.
」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」」＜第２章　物質の構成粒子＞（教p19-）