Fig. 13.
Composite spectrum of the spectroscopic binary star number 50. The spectrum of the star (in black) is compared to three standard star spectra of spectral type B0, B5, and B9 in blue, red, and green, respectively (described in Sect. 4.1), downgraded in resolution to match the MUSE data. The continuous colored line shows the original spectra, and the dash-dotted line shows the spectra after rotational broadening by 200 km s−1 was applied.
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