Table 4
Summary of matches between targets in the VLT-FLAMES Tarantula Survey (VFTS) and candidate young stellar objects (YSOs) from Gruendl & Chu (2009, “GC09”).
| Star | VFTS Sp. Type | Identification | Type | Δr | J | H | Ks | [3.6] | [4.5] | [5.8] | [8.0] | [24.0] |
| [VFTS] | [GC09] | [′′] | ||||||||||
|
|
||||||||||||
| 016 | O2 III-If∗ | 053708.79 − 690720.3 | CS | 0.5 | 13.39 | 13.37 | 13.35 | 12.99 | 12.20 | 10.61 | 8.73 | 3.82 |
| 178 | O9.7 Iab | 053751.03 − 690934.0 | CS | 0.1 | 12.84 | 12.83 | 12.81 | 12.71 | 12.48 | 11.69 | 9.76 | 3.87 |
| 320 | Be | 053821.10 − 690617.2 | CS | 0.4 | 15.19 | 14.98 | 14.64 | 13.21 | 12.86 | 11.85 | 10.04 | − |
| 345 | O9.7 III(n) | 053827.39 − 690809.0 | CS | 0.4 | 15.48 | 15.47 | 15.37 | 13.82 | 12.88 | 11.48 | 9.70 | − |
| 410 | Late O | 053834.77 − 690606.1 | C | 0.9 | Multiple components – see Walborn et al. (1999a, 2002) | |||||||
| 464 | B0: | 053839.24 − 690552.3 | C | 1.2 | 14.55 | 14.26 | 13.63 | 11.27 | 10.40 | 8.98 | 6.93 | − |
| 500 | Late O + late O | 053841.23 − 690259.0 | CS | 0.7 | 13.80 | 13.73 | 13.68 | 13.27 | 12.52 | 10.89 | 8.74 | 3.02 |
| 586 | O4 V((n))((fc))z | 053845.33 − 690251.6 | CS | 0.4 | 14.96 | 14.91 | 14.88 | 14.51 | 13.34 | 11.62 | 9.51 | 2.82 |
| 631 | O9.7 III(n) (SB1) | 053848.86 − 690828.0 | CS | 0.1 | 15.76 | 15.66 | 15.66 | 14.60 | 13.53 | 12.37 | 11.13 | − |
| 682 | WN5h | 053855.56 − 690426.5 | CS | 0.3 | 13.53 | 12.96 | 12.48 | 11.69 | 11.37 | 10.48 | 9.15 | − |
| 702 | O8.5 V (SB1) | 053858.42 − 690434.7 | C | 0.5 | 15.35 | 15.12 | 14.91 | 12.57 | 11.74 | 9.59 | 7.71 | − |
| 751 | O7-8 Vnnz | 053909.13 − 690128.7 | CS | 0.9 | 15.62 | 15.48 | 15.31 | 13.87 | 13.07 | − | 10.37 | 3.75 |
|
|
||||||||||||
| 152 | B2 V | 053746.64 − 690619.8 | SD | 0.4 | 14.66 | 14.47 | 14.30 | 14.05 | 13.99 | 13.26 | 11.76 | − |
| 323 | A5 II | 053821.78 − 691042.9 | SD | 0.1 | 14.26 | 14.07 | 13.91 | 13.81 | 13.86 | 13.15 | 11.57 | − |
| 641 | B0.5: I: | 053849.81 − 690643.3 | SD | 0.5 | 12.63 | 12.58 | 12.48 | 11.46 | 10.54 | 9.67 | 7.34 | 0.06 |
| 842 | Be | 053942.66 − 691151.6 | SD | 0.3 | 15.08 | 14.85 | 14.53 | 13.58 | 13.40 | − | 10.98 | − |
Notes. The fourth column is the source classification from GC09: “C” – candidate YSO; “CS” – probable YSO, but could possibly be a star; “SD” – stars with photometric contamination from diffuse emission. Near-IR photometry (JHKs) is from the IRSF catalogue (Kato et al. 2007), with mid-IR photometry from GC09. VFTS 410 = P93-409; the two major components were classified by Walborn et al. (2002) as O8.5 V and O9 V.
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