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Fig. 25.

image

Kinematics in NGC 300. Panel a: radial velocities determined for individual stars; panel b: radial velocities obtained from unresolved background tiles produced by PampelMUSE; panel c: radial velocities determined for PNe, errors coded with plot symbols (full circles <10 km s−1, thick rings <20 km s−1, thin rings >20 km s−1); panel d: reference velocity field reproduced from Hlavacek-Larrondo et al. (2011). The velocity field color coding is similar to, but differs slightly from, the color code for point sources in panels a and c.

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