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Figure 1:
Regression detection of a ![]() |
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Figure 2: Normalized Stokes I spectra of the three Herbig Ae stars. The individual spectra are displaced by 0.65 with respect to each other. |
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Figure 3: Stokes V/I spectra of the studied stars around the Ca II doublet. The individual spectra are shifted by 0.8 with respect to each other. |
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