Abstract
The photoabsorption of the imidogen (NH) radical is important in various astronomical and industrial processes. In particular, its photodissociation in the ultraviolet region is crucial for correct chemical modelling and dynamics. An updated spectroscopic model, named 2kNigHt, is presented for the 12 lowest electronic states of NH. This model is used to compute a new bound–bound line list up to 50 000 cm(Formula presented) for the four (Formula presented) N(Formula presented) H, (Formula presented) N(Formula presented) H, (Formula presented) N(Formula presented) H, and (Formula presented) N(Formula presented) H isotopologues. Temperature-dependent photoabsorption, continuum photoabsorption, and photodissociation cross-sections, as well as associated photolysis rates under several important radiation fields, are computed. These cross-sections cover wavelengths longer than the hydrogen Ly(Formula presented) line for temperatures up to 10 000 K. All results are made available in the ExoMol and ExoPhoto databases.
| Original language | English |
|---|---|
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 548 |
| Issue number | 3 |
| DOIs | |
| State | Published - May 2026 |
Keywords
- astrochemistry
- ISM: molecules
- molecular data
- planets and satellites: atmospheres
- stars: atmospheres
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