Structure of the outer Galactic disc with Gaia DR2

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Fig. 21.

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Comparison of line of nodes for our model (based on Eq. (11)) with other works. We use two different methods to plot the line of nodes for our work. First, we plot the angle ϕ_w for Eq. (12). Another method is to use the Eq. (11) to find the value of the angle ϕ when z_w = 0.

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