Consistent dust and gas models for protoplanetary disks: II. Chemical networks and rates
Aims: We aim to define a small and large chemical network which can be used for the quantitative simultaneous analysis of molecular emission from the near-IR to the submm. We also aim to revise reactions of excited molecular hydrogen, which are not included in UMIST, to provide a homogeneous databas...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2017-11, Vol.607, p.A41 |
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