Table 5: Final core masses at the pre-supernova stage for different models of rotating stars at solar metallicity. Note that we use $M_{\rm {Si}}$ at the end of central Si-burning for the value of $M_{\rm {Fe}}$ as discussed in the text.
$M_{\rm {ZAMS}}$ 15 F15B (HLW) E15 (HLW) 20 F20B (HLW) E20 (HLW) 25 E25 (HLW)

$M_{\rm {total}}$ 10.316 12.89 10.86 8.763 14.76 11.00 10.042 5.45

$M_{\alpha}^{01}$ 5.604 3.88 5.10 8.567 5.99 7.71 10.042 5.45

$M_{\rm {CO}}^{01}$ 3.325 2.01 3.40 5.864 2.75 5.01 7.339 4.07

$M_{\rm {Fe}}^{50}$ 2.036 1.38 1.46 2.245 1.36 1.73 2.345 1.69

**Table 5:** Final core masses at the pre-supernova stage for different models of rotating stars at solar metallicity. Note that we use $M_{\rm {Si}}$ at the end of central Si-burning for the value of $M_{\rm {Fe}}$ as discussed in the text.
$M_{\rm {ZAMS}}$	15	F15B (HLW)	E15 (HLW)	20	F20B (HLW)	E20 (HLW)	25	E25 (HLW)
$M_{\rm {total}}$	10.316	12.89	10.86	8.763	14.76	11.00	10.042	5.45
$M_{\alpha}^{01}$	5.604	3.88	5.10	8.567	5.99	7.71	10.042	5.45
$M_{\rm {CO}}^{01}$	3.325	2.01	3.40	5.864	2.75	5.01	7.339	4.07
$M_{\rm {Fe}}^{50}$	2.036	1.38	1.46	2.245	1.36	1.73	2.345	1.69

Source LaTeX | All tables | In the text