Table 11
Properties of supergiants with a projected rotational velocity of more than 100 km s-1.
| Star | ST | vesini | T eff | log g |
|
log L/ L⊙ | Ms/ M⊙ | Me/ M⊙ | log t |
| km s-1 | K | cm s-2 | |||||||
|
|
|||||||||
| VFTS 060 | B1.5 II-Ib((n)) | 129 | 19 500 | 2.65 | ≤6.9 | 4.82 | 8 | 23 | 6.84 |
| VFTS 293 | B2 III-II(n)e | 125 | 20 000 | 3.00 | ≤6.9 | 4.84 | 16 | 15 | 7.08 |
| VFTS 826 | B1 IIn | 222 | 23 500 | 3.25 | 6.80 | 4.85 | 15 | 16 | 7.04 |
| NGC2004-13 | B2 II | 145 | 21 500 | 3.20 | 6.85 | 4.94 | 24 | 14 | 7.13 |
|
|
|||||||||
| VFTS 450 | O9.7 III: +O7:: | 123 | 27 000 | 3.00 | 7.49 | 5.67 | 33 | 39 | 6.59 |
| VFTS 687 | B1.5 Ib((n)) Nwk | 123 | 20 000 | 2.65 | 6.94 | 4.95 | 9 | 25 | 6.80 |
| VFTS 829 | B1.5-2 II | 138 | 20 500 | 2.90 | ≤7.1 | 4.78 | 10 | 18 | 6.96 |
| NGC2004-15 | B1.5 II | 165 | 23 000 | 3.15 | 6.95 | 4.96 | 22 | 17 | 6.98 |
| NGC2004-20 | B1.5 II | 145 | 23 000 | 3.20 | 7.46 | 4.91 | 25 | 16 | 7.01 |
Notes. The VFTS targets have been taken from Tables 4 and 7. The FLAMES-I estimates (identified using the associated cluster, either N11 or NGC 2004) have been taken from Hunter et al. (2007) and Trundle et al. (2007) or have been estimated using the same methodology as for the Tarantula targets. The luminosities and masses are in units of the solar value. The single stellar candidates are listed first followed by the binaries.
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