Progenitors of low-mass binary black-hole mergers in the isolated binary evolution scenario

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Volume 649 (May 2021)

A&A, 649 (2021) A114

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Table A.1.

Summary of MESA runs performed with α_CE = 2.0.

ϵ	Z	Runs	BBH	BBH (< t_Hubble)	GW170608	GW151226	M_i, 1 [M_⊙]	M_i, 2 [M_⊙]	a_i [R_⊙]
0.6	0.0001	595	455	111	14	25	21–35	16–34	27–150
	0.001	1727	436	120	16	8	21–45	14–36	30–300
	0.004	1245	419	95	7	7	23–45	18–42	30–200
	0.007	1854	503	60	11	5	27–57	20–44	36–200
	0.015	5223	1520	81	2	1	29–89	26–78	36–200

0.4	0.0001	636	497	115	7	10	21–37	18–34	27–186
	0.001	1669	476	76	5	8	21–45	20–36	30–200
	0.004	2223	697	54	4	4	25–53	20–48	33–200
	0.007	2453	681	34	9	15	29–65	24–58	36–200
	0.015	3549	1382	192	31	59	29–85	26–78	43–200

0.2	0.0001	481	349	51	5	6	23–39	20–34	30–122
	0.001	1019	261	24	3	3	25–47	22–46	30–100
	0.004	1221	424	21	7	3	29–61	24–42	36–91
	0.007	2750	961	59	13	17	29–83	26–50	36–150
	0.015	5019	2996	35	0	0	36–91	26–58	36–150

0.0	0.0001	137	85	0	0	0	29–37	24–32	30–63
	0.001	348	207	0	0	0	29–41	26–34	36–100
	0.004	744	472	0	0	0	37–49	26–46	36–100
	0.007	1102	554	0	0	0	43–57	30–54	36–150
	0.015	2135	1405	0	0	0	43–79	32–56	30–2000

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