Fig. 5

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Changes in the abundances of gas- and ice-phase radicals over time in a dark cloud. The solid lines represent the results obtained using the BE values from Garrod (2013, “G”), while the dashed curves represent the results obtained using our calculated BE values (“G+S”). The filled curve around the calculated BE curves shows the abundances when the errors on the calculated BEs are taken into account, as presented in Table 2.
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