25 years of XMM-Newton observations of the Sgr A complex - 3D distribution and internal structure of the clouds

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Fig. 9

Same as Fig. 8, but the whole CMZ region is shown. The dashed line is the dynamical model proposed by Kruijssen et al. (2015). Most of the molecular clouds in the CMZ should roughly lie on the ellipsoid. Regardless of the scenario, the Sgr A complex appears to be located at smaller radii than the nuclear ring.

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