The Smallest Scale of Hierarchy Survey (SSH) - III. Dwarf-dwarf satellite merging phenomena in the low-mass regime

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Fig. 6

Same as Figure 5 for UGC 6456. The field of view here is ~4.5′ × 7.1′, or ~5.6 × 8.9 kpc², and the HI contours correspond to [0.1, 0.5, 1, 5.2, 10, and20] ×10²⁰ atoms/cm². TheHI data are taken from the VLA program LITTLE THINGS (Hunter et al. 2012).

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