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Table 2

Limits for the dipolar field strength obtained through Bayesian statistical considerations.

STAR
Of?p:
AzV 220 2325 N 8825 N
SMC 159-2 12 125 m 10725 N
SMC 159-2 (relative) 10 075 s 7275 N
SMC 159-2 (absolute) 11 275 vs 9825 N
LMCe 136-1 2825 N 1375 N
LMCe 136-1 (relative) 3225 N 1475 N
LMCe 136-1 (absolute) 4625 N 2275 N
LMC 164-2 3775 N 7975 N
LMC 164-2 (relative) 3775 N 7975 N
LMC 164-2 (absolute) 6725 N 2525 N

OB supergiants:
Mk 42 (VMS) 3725 N 1825 N
VFTS 526 7975 N 5725 N
Mk37Wa (VMS) 6925 N 8825 N
VFTS 291 4275 N 6175 N
VFTS 458 2075 N 3525 N

BA giants:
NGC 346 ELS 1080 9475 N 5375 N
NGC 346 ELS 19 7025 N 6075 N

OB dwarfs:
VFTS 441 5875 N 4875 N
VFTS 500 7075 N 18925 w
VFTS 506 (VMS) 2474 N 3575 N
VFTS 586 12 285 N 5565 N
VFTS 621 (VMS) 1525 N 1275 N
VFTS 589 9025 N 7225 N
AzV 55 1025 N 975 N
AzV 66 1325 N 2075 N
2dFS 5037 8925 N 4375 N
2dFS 5038 1675 N 1225 N
NGC 346 ELS 27 12 975 N 4475 N
NGC 346 ELS 68 6525 N 5525 N
NGC 346 ELS 100 5075 N 8625 N
NGC 346 ELS 103 3275 N 16675 N

Cool supergiants:
W60 D24 175 N 225 N
RM 1-546 775 N 775 N
SkKM 179 3025 N 575 N
VFTS 341 1075 N 625 N
CPD−69 463 1175 N 775 N

WR:
VFTS 507 925 N 1425 N
VFTS 509 1175 N 1825 N
R 136c (VMS) 12 675 N 5575 N
VFTS 682 (VMS) 2975 N 3075 N

Notes. Column 2 reports the value, and the flag of Col. 3 means no (N), weak (w), moderate (m), strong (s), or very strong (vs) evidence for the presence of a magnetic field. Columns 4 and 5 as Cols. 2 and 3, but for the null field values. The meaning of relative and absolute refers to results obtained assuming that the star’s rotation period is known, as explained in the text.

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