SR 12 c's Hα profile is asymmetric, blueshifted, and variable on hourly timescales, consistent with magnetospheric accretion but not ruling out a boundary-layer plus failed-wind model.
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Asymmetric, variable H$\alpha$ line profile in planetary mass object SR 12 c
SR 12 c's Hα profile is asymmetric, blueshifted, and variable on hourly timescales, consistent with magnetospheric accretion but not ruling out a boundary-layer plus failed-wind model.