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Evolution of massive Be and Oe stars at low metallicity towards the Long Gamma Ray bursts\footnote{Based on ESO runs 069.D-0275(A), 072.D-0245(A) and (C).}

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Academic year: 2021

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Figure 1: Comparison of LGRBs progenitors area (dashed) at Z SM C at the ZAMS with categories of SMC Be/Oe stars (grey-plain ABCDE areas)

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