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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