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Fig. 12


Spectral ratios of limb-transit to out-of-transit for a low-mass star with Teff = 3000 K. The spectral ratio for a star with Teff = 4000 K is also plotted for comparison. One can see a different behaviour of the line wing for 3000 K. The wavelength range here is larger than in Fig. 8 in order to give a clearer view of the broad line profile.

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