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Fig. 6.

Deblending of the extremely faint emission line star (A) from an unresolved group of K stars (C). For an explanation, see Fig. 5 and text below. The insert spectrum covers the wavelength range 6200 … 7000 Å, flux is plotted in units of erg cm−2 s−1 Å−1 (continuum background not subtracted).
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