Failed supernova explosions increase the duration of star formation in globular clusters

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Table A.1

The deduced masses, metallicities, numbers of CCSNe and times when SF ends for 55 Galactic GCs.

Name	M_ini [10⁵M_⊙]	$M_{ini}^{old} [10^{5} M_{⊙}]$ $M_{{\rm{ini}}}^{{\rm{old}}}\left[ {{{10}^5}{M_ \odot }} \right]$	[Fe/H]	N_SN	$t_{all}^{SF}$ $t_{{\rm{all}}}^{{\rm{SF}}}$ [Myr]	t^SF	$t_{W 18}^{SF}$ $t_{{\rm{W}}18}^{{\rm{SF}}}$ [Myr]	$t_{W 18, 0.5 M_{gas}}^{SF}$ ${t_{{\rm{W}}18,0.5{{\rm{M}}_{{\rm{gas}}}}}^{{\rm{SF}}}}$ [Myr]
47 Tuc	36.55	27.50	−0.747	4.31 × 10³	3.6	12.1	7.8	4.1
NGC 288	6.86	17.79	−1.226	3.01 × 10²	3.4	10.7	4.0	3.4
NGC 362	27.66	93.75	−1.213	2.51 × 10³	3.5	11.2	7.3	3.9
NGC 1851	26.92	136.44	−1.157	1.72 × 10³	3.5	10.9	4.0	3.4
NGC 1904	21.68	142.09	−1.550	3.29 × 10²	3.4	10.0	3.4	3.4
NGC 2419	104.06	42.97	−2.095	5.34 × 10²	3.4	9.8	3.4	3.4
NGC 2808	64.73	127.73	−1.120	3.43 × 10³	3.4	10.8	3.9	3.4
NGC 3201	5.32	4.32	−1.496	1.49 × 10²	3.4	10.2	3.8	3.4
NGC 4590	5.42	3.72	−2.255	3.19 × 10¹	3.4	9.8	3.4	3.4
NGC 4833	24.91	118.88	−2.070	5.50 × 10¹	3.4	9.7	3.4	3.4
NGC 5024	20.49	11.69	−1.995	2.95 × 10²	3.4	9.9	3.4	3.4
NGC 5053	2.98	2.20	−2.450	8.67 × 10⁰	3.4	9.7	3.4	3.4
NGC 5139	376.26	178.36	−1.647	4.89 × 10⁴	3.4	11.4	7.0	3.4
NGC 5272	16.46	12.17	−1.391	1.31 × 10³	3.5	11.0	7.2	3.9
NGC 5286	29.91	68.41	−1.727	1.16 × 10³	3.4	10.2	3.4	3.4
NGC 5466	2.20	2.07	−1.865	4.52 × 10¹	3.4	10.0	3.8	3.4
NGC 5634	10.81	9.09	−1.869	2.38 × 10²	3.4	10.0	3.4	3.4
NGC 5694	19.21	13.10	−2.017	1.70 × 10²	3.4	9.8	3.4	3.4
NGC 5824	52.40	23.77	−2.174	4.07 × 10²	3.4	9.8	3.4	3.4
NGC 5904	18.13	17.63	−1.259	8.18 × 10²	3.4	10.6	3.9	3.4
NGC 5986	43.26	253.81	−1.527	1.57 × 10³	3.4	10.3	3.4	3.4
NGC 6093	94.42	1467.87	−1.789	4.29 × 10²	3.4	9.8	3.4	3.4
NGC 6121	25.57	325.37	−1.166	1.74 × 10³	3.5	11.0	4.1	3.4
NGC 6139	28.99	64.92	−1.593	4.88 × 10²	3.4	10.0	3.4	3.4
NGC 6171	11.62	75.02	−0.949	1.23 × 10³	3.7	11.9	7.8	4.1
NGC 6205	31.91	47.26	−1.443	2.34 × 10³	3.4	10.8	4.0	3.4
NGC 6218	6.80	16.64	−1.315	1.91 × 10²	3.4	10.3	3.9	3.4
NGC 6229	15.26	22.35	−1.129	9.98 × 10²	3.5	11.0	7.2	3.9
NGC 6254	13.82	27.25	−1.559	3.74 × 10²	3.4	10.2	3.4	3.4
NGC 6266	63.96	224.31	−1.075	4.41 × 10³	3.5	11.0	4.0	3.5
NGC 6273	56.62	95.00	−1.612	4.55 × 10³	3.4	10.8	3.9	3.4
NGC 6341	33.17	92.11	−2.239	3.19 × 10²	3.4	9.8	3.4	3.4
NGC 6362	7.31	15.32	−1.092	2.01 × 10²	3.4	10.5	3.9	3.4
NGC 6366	4.01	17.45	−0.555	1.59 × 10³	7.7	18.6	17.7	12.6
NGC 6388	61.01	110.26	−0.428	2.46 × 10⁴	5.2	16.2	14.7	10.3
NGC 6397	6.86	12.37	−1.994	3.89 × 10¹	3.4	9.8	3.4	3.4
NGC 6402	76.64	362.45	−1.130	6.02 × 10³	3.5	11.1	4.0	3.4
NGC 6441	65.26	126.76	−0.334	4.79 × 10⁴	8.2	22.4	−	13.6
NGC 6535	12.45	103.20	−1.963	9.48 × 10¹	3.4	9.8	3.4	3.4
NGC 6553	16.67	49.39	−0.151	1.11 × 10⁴	10.4	21.9	−	14.0
NGC 6569	15.08	36.03	−0.867	2.25 × 10³	3.9	12.7	10.0	7.6
NGC 6626	49.46	452.45	−1.287	3.84 × 10³	3.4	11.0	4.0	3.4
NGC 6656	23.94	19.75	−1.803	1.01 × 10³	3.4	10.3	3.8	3.4
NGC 6681	21.49	149.57	−1.633	2.80 × 10²	3.4	9.9	3.4	3.4
NGC 6715	113.80	50.19	−1.559	1.18 × 10⁴	3.4	11.1	7.0	3.4
NGC 6752	13.00	14.72	−1.583	2.31 × 10²	3.4	10.0	3.4	3.4
NGC 6809	16.27	36.99	−1.934	1.70 × 10²	3.4	9.8	3.4	3.4
NGC 6838	2.86	4.46	−0.736	4.10 × 10²	4.5	13.2	11.5	7.9
NGC 6864	23.52	33.22	−1.164	1.90 × 10³	3.5	11.2	7.3	3.9
NGC 7078	30.98	19.26	−2.287	1.70 × 10²	3.4	9.8	3.4	3.4
NGC 7089	64.36	417.15	−1.399	1.08 × 10³	3.4	10.1	3.4	3.4
NGC 7099	14.02	35.18	−2.356	4.57 × 10¹	3.4	9.7	3.4	3.4
Terzan 1	177.07	5089.44	−1.263	7.14 × 10³	3.4	10.5	3.4	3.4
Terzan 5	40.85	136.44	−0.092	2.10 × 10⁵	−	−	−	−
Terzan 8	188.04	4604.79	−2.255	2.06 × 10³	3.4	9.8	3.4	3.4

Notes. The columns from left to right are: the name of the GC, the initial mass, M_ini, the initial mass computed by Wirth et al. (2022), $M_{ini}^{old}$ $M_{{\rm{ini}}}^{{\rm{old}}}$ , the metallicity, [Fe/H], the number of CCSNe, N_SN, the time SF ends assuming: 1. all stars above 8M_⊙ explode as CCSNe, $t_{all}^{SF}$ $t_{{\rm{all}}}^{{\rm{SF}}}$ , 2. all CCSNe of stars above 20 M_⊙ fail, t^SF, 3. model W18 from Sukhbold et al. (2016) and 4. model W18 from Sukhbold et al. (2016) with only half of the total gas mass left.

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