Fig. 4.
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Integrated H I spectra of ESO444–G084 (left) and [KKS2000]23 (right) from MeerKAT (black solid line) and HIPASS (black dashed line, Koribalski et al. 2004). The black arrow on each figure shows the kinematic systemic velocity of each galaxy derived in Section 5. The horizontal dashed grey lines indicate the zero level. These profiles are derived from the high-resolution data.
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