Abundant Hydrocarbons
Abundant Hydrocarbons
Using the zero-dimensional LTE SLAB-models that are part of ProDi...
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CAI formation in the early Solar Nebula
CAI formation in the early Solar Nebula
  This paper proposes a pathway to form mm-sized, pure, and...
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Fitting the EX Lupi JWST line & continuum spectrum with ProDiMo
Fitting the EX Lupi JWST line & continuum spectrum with ProDiMo
Based on an improved ProDiMo version, we developed a disc model f...
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ALMA gaps
ALMA gaps
ProDiMo can predict continuum images and molecular line channel m...
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ice absorption
ice absorption
One of the latest developments of ProDiMo is to include ice opaci...
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Disk winds
Disk winds
We use hydrodynamic photoevaporative disk-wind models and post-pr...
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Chemical processes
Chemical processes
ProDiMo's goal is to model the chemistry and heating/cooling bala...
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Heating and Cooling
Heating and Cooling
At each point in the disk, ProDiMo solves the gas heating and coo...
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surface chemistry
surface chemistry
ProDiMo is now able to take into account surface chemical process...
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phyllosilicates
phyllosilicates
The hydration of rocks can optionally be included as a time-depen...
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Chemical rate networks
Chemical rate networks
With ProDiMo you can use various standard chemical rate networks ...
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IR molecular line emission spectra
IR molecular line emission spectra
ProDiMo allows you to generate mid-IR molecular emission line spe...
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CO ro-vibrational emission lines
CO ro-vibrational emission lines
ProDiMo can predict high-resolution infrared line spectra emitted...
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FU Ori outbursts
FU Ori outbursts
In FU Ori type outbursts, driven by episodic accretion, the stellar lu...
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ProDiMo can predict high-resolution infrared line spectra emitted from the inner disk, including CO fundamental and overtones.  In case of CO, the user can specify the number of vibrational, rotational, and electronic states to be included into the non-LTE model, see (Thi+2013) for details.  The latter allows us to include the effects via fluorescent pumping. The example figure shows the CO fundamental spectrum for BP Tau (Woitke+2019, PASP 131, 4301). The strong CO lines appear asymmetric in the model because of underlying H2O lines.