Fig. 10.
Two-dimensional velocity map in the Hα line of the central 40″ × 40″ of NGC 185, constructed from three slit positions for high-resolution spectra, with objects denoted as in Fig. 2. Contours denote Hα intensity from narrowband imaging. Assuming that heliocentric velocity of the galaxy is −203.8 km s−1 (McConnachie 2012), we observe the receding side of shells VIEM 8 and VIEM 9.
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