Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at Small Magellanic Cloud metallicity

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Volume 687 (July 2024)

A&A, 687 (2024) A290

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Table 3.

O-type giants and supergiants from Bouret et al. (2021).

Star	Sp. type	T_eff	log g	L_*	v sin i	Y_He	ϵ(N)	log(N/C)

		[kK]		[L_⊙]	[km s⁻¹]	Mass fraction	By number
AV 15	O6.5I(f)	39.0	3.61	5.83	120.00	0.285	7.78 ± 0.16	$0 . 78_{- 0.17}^{+ 0.23}$ $0.78_{-0.17}^{+0.23}$
AV 43	B0.5III	28.5	3.37	5.13	200.00	0.374	$7 . 45_{- 0.20}^{+ 0.25}$ $7.45_{-0.20}^{+0.25}$	$- 0 . 03_{- 0.21}^{+ 0.43}$ $-0.03_{-0.21}^{+0.43}$
AV 47	O8III((f))	35.0	3.75	5.44	60.00	0.285	7.08 ± 0.15	$- 0 . 61_{- 0.15}^{+ 0.20}$ $-0.61_{-0.15}^{+0.20}$
AV 69	OC7.5III((f)	33.9	3.50	5.61	70.00	0.285	6.34 ± 0.17	$- 1 . 22_{- 0.19}^{+ 0.27}$ $-1.22_{-0.19}^{+0.27}$
AV 75	O5.5I(f)	38.5	3.51	5.94	120.00	0.324	$8 . 00_{- 0.13}^{+ 0.15}$ $8.00_{-0.13}^{+0.15}$	$1 . 00_{- 0.15}^{+ 0.29}$ $1.00_{-0.15}^{+0.29}$
AV 77	O7III	37.5	3.74	5.40	150.00	0.374	$7 . 08_{- 0.05}^{+ 0.11}$ $7.08_{-0.05}^{+0.11}$	$- 0 . 10_{- 0.15}^{+ 0.19}$ $-0.10_{-0.15}^{+0.19}$
AV 83	O7Iaf+	32.8	3.26	5.54	80.00	0.444	8.41 ± 0.20	$0 . 83_{- 0.18}^{+ 0.28}$ $0.83_{-0.18}^{+0.28}$
AV 95	O7III((f))	38.0	3.70	5.46	53.00	0.285	7.60 ± 0.11	$0 . 30_{- 0.13}^{+ 0.16}$ $0.30_{-0.13}^{+0.16}$
AV 170	O9.7III	30.5	3.41	5.14	70.00	0.324	$7 . 70_{- 0.10}^{+ 0.16}$ $7.70_{-0.10}^{+0.16}$	$0 . 40_{- 0.14}^{+ 0.22}$ $0.40_{-0.14}^{+0.22}$
AV 232	O7Iaf+	33.5	3.16	5.89	75.00	0.444	8.36 ± 0.20	$0 . 86_{- 0.18}^{+ 0.28}$ $0.86_{-0.18}^{+0.28}$
AV 307	O9III	30.0	3.50	5.15	60.00	0.324	7.56 ± 0.18	$0 . 18_{- 0.20}^{+ 0.30}$ $0.18_{-0.20}^{+0.30}$
AV 327	O9.7I	30.0	3.12	5.54	95.00	0.374	$8 . 08_{- 0.25}^{+ 0.20}$ $8.08_{-0.25}^{+0.20}$	$0 . 78_{- 0.21}^{+ 0.28}$ $0.78_{-0.21}^{+0.28}$
AV 439	O9.5III	31.0	3.54	5.16	260.00	0.308	7.90 ± 0.20	$0 . 28_{- 0.20}^{+ 0.29}$ $0.28_{-0.20}^{+0.29}$

Notes. The helium abundances, originally given by number, were readapted as mass fractions for the purposes of this work.

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