Stellar population of the superbubble N 206 in the LMC - II. Parameters of the OB and WR stars, and the total massive star feedback

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Table 2

Main diagnostics used in our spectral fitting process.

Parameter	O stars	Early B stars	Late B stars
T_*	He I/He II line ratios	Si III/Si IV line ratios	Si II/Si III, Mg II/He I line ratios
log g_*	Hγ and Hδ line wings	Hγ and Hδ line wings	Hγ and Hδ line wings
Ṁ	Hα, He II 4686, Si IV 1393–1403	Hα, He II 4686, Si IV 1393–1403	Hα, He II 4686, Si IV 1393–1403
	P V 1118–1128, C IV 1169, C III 1176	C IV 1548–1551
	C IV 1548–1551
v_∞	Hα, N V 1238–1242, C IV 1548–1551	Hα, C IV 1548–1551	Hα, Si IV 1393–1403
	Si IV 1393–1403, P V 1118–1128	Si IV 1393–1403
v sini	He I lines, N III 4510–4525	He I lines, N III 4641	He I lines, C II 4267
	Si IV 4089–4116	Si III 4552–4575, O II 4649	Mg II 4481
v_rad	He I and He II lines	He I lines, Si III 4552–4575	He I lines, C II 4267, Mg II 4481

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