Small-scale physical and chemical structure of diffuse and translucent molecular clouds along the line of sight to Sgr B2

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Fig. 24

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Same as Fig. 23, but for ¹³CO 1–0. The ALMA spectrum is resampled to the spectral resolution of the Mopra spectrum. The dashed lines mark emission peaks that match well absorption features of the EMoCA spectrum outside the velocity range of the Sgr B2 envelope.

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