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Fig. 3


Left: oscillation of the Sun governed by Eq. (17) in MD. We used z(0) = 30 pc and vz(0) = 7.25 km s-1 as the initial conditions of the Sun’s motion. Middle: local “total matter density” ϱ = ϱb + ϱph, as experienced by the oscillating Sun. Right: local PMD, as experienced by the oscillating Sun.

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