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Fig. 12

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FLAMES-Giraffe spectroscopy of ten candidate YSOs from Gruendl & Chu (2009), as summarised in Table 4. Strong nebular lines have been truncated as indicated. The He II lines identifed in VFTS 500 (a double-lined spectroscopic binary) are: λλ4200, 4542, 4686; He I lines identified in VFTS 631 are: λλ4009, 4026, 4144, 4388, 4471, 4713.

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