The different progenitors of type Ib, Ic SNe, and of GRB

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Table 4:

Mass ranges for various supernova progenitors, supernova types, and compact remnants at different metallicities (in ${M}_\odot$ ).
Z	SG	WNL	WNE	WC	WO	Type II	Type Ib	Type Ic	NS	BH
Reference case
0.004	8 - 32	32 - 54	-	54 - 59;114 - 120	59 - 114	8 - 54	54 - 59	59 - 120	8 - 29	29 - 120
0.008	8 - 25	25 - 30	-	30 - 41; 113 - 120	41 - 113	8 - 30	-	30 - 120	8 - 29	29 - 120
0.020	8 - 23	23 - 26	26 - 29	29 - 120	-	8 - 25	25 - 39	39 - 120	8 - 35	35 - 120
0.040	8 - 20	20 - 20.5	20.5 - 22	22 - 120	-	8 - 20.5	20.5 - 25	25 - 120	8 - 120	-1

(1) At this metallicity, only the $40~ {M}_\odot$ model produces a BH. Note: The SN type is given for $m^{\rm min}_{\rm H}=0$ , $m^{\rm min}_{\rm He}=0.6$ and supposing that an SN occurs even when a BH is formed (see text for more details).

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