The Arches cluster revisited - II. A massive eclipsing spectroscopic binary in the Arches cluster

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Fig. 6

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C IV 2.079 μm line at threephases: in black, near secondary eclipse (phase 0.550); in blue and red, near quadratures (phases 0.324 and 0.760). Although the line is faint and noisy, we may observe that the main peak moves in anti-phase with the other lines (e.g. Figs. 2 and 3).

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