Fig. 11.
MUSE spectrum of A5 supergiant B11 from the sample of Bresolin et al. (2002), seen in field (b), ID25. This star has a V magnitude of 19.95. The MIUSCAT fit is plotted in orange with an offset for clarity. Wavelengths in units of Å, flux in units of 10−20 erg cm−2 s−1 Å−1. The reference wavelengths of a number of absorption lines (hydrogen Balmer and Paschen series, helium lines) are indicated.
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