Fig. 9.
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Projected distance to nearest massive galaxy. All dwarfs in our observed area are shown as the filled-black histogram. H I-detected LTDs are shown in the blue-filled histogram, LTDs with disturbed H I are shown by the dashed green-filled histogram and H I-undetected LTDs are the open orange histogram. There are no H I-detected LTDs within a projected distance of 100 kpc to their nearest massive galaxy, implying that massive galaxies play an active role in the removal of H I from LTDs.
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