Evolutionary models for the very massive stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud

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Volume 700 (August 2025)

A&A, 700 (2025) A186

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Table C.2.

Same as Table C.1, but using the SB models.

R136a1	SB scheme
v_rot, ini	M_ini	M_curr	t	$χ_{total}^{2}$ $\chi^2_{\rm total}$
100	408, 425	347, 351 (350 $_{- 44}^{+ 53}$ $^{+53}_{-44}$ )	0.83, 0.94 (0.92±0.16)	7.80, 7.01
200	404, 397	341, 330 (330 $_{- 42}^{+ 52}$ $^{+52}_{-42}$ )	0.84, 0.93 (0.93±0.15)	5.94, 5.37
300	328, 329	272, 276 (299 $_{- 39}^{+ 53}$ $^{+53}_{-39}$ )	1.11, 1.05 (0.97±0.16)	3.77, 3.47
400	330, 316	276, 264 (282 $_{- 34}^{+ 53}$ $^{+53}_{-34}$ )	1.07, 1.12 (1.00±0.16)	2.40, 2.27
500	301, 303	255, 255 (280 $_{- 33}^{+ 51}$ $^{+51}_{-33}$ )	1.07, 1.11 (1.00±0.16)	2.04, 1.95

R136a2

100	> 550 (716, 724)	196, 195 (195 $_{- 33}^{+ 38}$ $^{+38}_{-33}$ )	1.44, 1.45 (1.50±0.10)	3.85, 3.58
200	> 570 (728, 729)	191, 193 (194 $_{- 32}^{+ 38}$ $^{+38}_{-32}$ )	1.46, 1.45 (1.50±0.10)	3.31, 3.30
300	> 520 (720, 630)	183, 197 (192 $_{- 32}^{+ 38}$ $^{+38}_{-32}$ )	1.47, 1.46 (1.50±0.10)	4.65, 4.47
400	> 510 (687, 735)	189, 195 (193 $_{- 32}^{+ 38}$ $^{+38}_{-32}$ )	1.46, 1.45 (1.50±0.11)	4.54, 4.39
500	> 500 (675, 640)*m	191, 202 (193 $_{- 32}^{+ 38}$ $^{+38}_{-32}$ )	1.48, 1.45 (1.50±0.11)	4.49, 4.02

R136a3

100	> 510 (715, 721)	173, 187 (184 $_{- 23}^{+ 53}$ $^{+53}_{-23}$ )	1.50, 1.47 (1.52±0.11)	4.00, 3.81
200	> 510 (725, 725)	185, 186 (185 $_{- 34}^{+ 41}$ $^{+41}_{-34}$ )	1.47, 1.46 (1.53±0.13)	3.58, 3.57
300	> 530 (789, 630)	192, 182 (183 $_{- 34}^{+ 46}$ $^{+46}_{-34}$ )	1.45, 1.49 (1.52±0.12)	4.58, 4.25
400	> 510 (769, 645)	172, 182 (188 $_{- 36}^{+ 35}$ $^{+35}_{-36}$ )	1.50, 1.49 (1.52±0.13)	4.51, 4.25
500	> 530 (635, 636)*m	175, 188 (191 $_{- 38}^{+ 47}$ $^{+47}_{-38}$ )	1.51, 1.48 (1.54±0.14)	4.24, 4.12

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