Fig. 1

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APEX observations of several transitions of N2H+ and N2D+ towards the dust peak of the pre-stellar core I16293E (black histograms) and results of the LOC non-LTE radiative transfer model (red curve). The physical model of I16293E computed from Herschel SPIRE and PACS data is shown in the upper right panel. The black curve (left y-axis) shows the total volume density , the red curve (right y-axis) shows the dust temperature, and the vertical dashed line indicates the 3000 au (21″) inner radius of the infalling envelope (see Sect. 3).
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