Fig. 5.
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Emission profile of the whole body of WLM from three major HI observations. The GBT observations are from the same data cube used in Ianjamasimanana et al. (2020), and little things VLA data are from Hunter et al. (2012). All observations were masked by SoFiA-2 and a common velocity range was set. Velocities are in the rest frame.
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