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Fig. 11


Combined FLAMES-ARGUS spectrum of VFTS 1003, a newly discovered B[e]-type star. There appears to be weak stellar absorption at He I λλ4009, 4026, 4388, 4471, combined with weak nebular emission components, particularly at λ4471. In addition to the Balmer lines, the identified lines are [S II] λ4069; [O III] λ4363; Fe II λλ4173, 4179, 4233, 4303, 4352, 4385, 4481, 4491, 4508, 4515, 4520-23, 4549, 4556; [Fe II] λλ4244, 4277, 4287, 4358-59, 4414-16.

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