Misalignment of the outer disk of DK Tau and a first look at its magnetic field using spectropolarimetry

Open Access

Fig. 3.

Average line-of-sight magnetic field B_los as derived from the photospheric absorption lines and veiling over time, shown folded in phase with the derived 8.2 day period, for the 2010 (left panel) and 2012 (right panel) datasets. Different colors and symbols represent different rotation cycles.

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