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Fig. B.1


Variation of emission line fluxes with date after outburst (see Sect. 2): Hα (diamond); Hβ (triangle); [Ne III] 3869 Å (plus); [N II] 5755 Å (cross); He I 5876 Å (square). The last date is from Munari (2012). Fluxes are not corrected for E(B − V).

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