Fig. 1.
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Comparison of the normalized observed spectrum of J1022−3414 and those of two known LP 40−365 type stars from Raddi et al. (2019) retrieved from the ESO archive. The two known LP 40−365 type stars have been smoothed to the same resolution as J1022−3414 and the wavelengths are at rest. Lines of magnesium, neon, and oxygen are marked. J1022−3414 shows broader lines than the other two.
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