GaiaUnlimited: The old stellar disc of the Milky Way as traced by the red clump

Open Access

Fig. 26

Posterior probability distributions for two warp parameters (R_w,h_w0) assuming Model 2 (Table 4) applied to ɡdr3wise[RC]. We show four cases where the other two warp parameters (ϕ_w,a_w) have been fixed. The residuals for these are shown in Fig. H.1.

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