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Fig. 5
Results for the self-regulated disk models with an initially atomic gas (Table 6). The species abundances and heating/cooling rates are given for the HS0 (self-regulated disk with central source of 1 M⊙ and an accretion rate of 10-1 M⊙ yr-1). We refer to the caption of Fig. 3 for the description of the panels.
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