ASCL Code Record
[ascl:1809.009]
NEBULA: Radiative transfer code of ionized nebulae at radio wavelengths
NEBULA performs the radiative transfer of the 3He+ hyperfine transition, radio recombination lines (RRLs), and free-free continuum emission through a model nebula. The model nebula is composed of only H and He within a three-dimension Cartesian grid with arbitrary density, temperature, and ionization structure. The 3He+ line is assumed to be in local thermodynamic equilibrium (LTE), but non-LTE effects and pressure broadening from electron impacts can be included for the RRLs. All spectra are broadened by thermal and microturbulent motions.
- Code site:
- https://doi.org/10.20356/C4X08M
- Used in:
- https://ui.adsabs.harvard.edu/abs/2018AJ....156..280B https://ui.adsabs.harvard.edu/abs/2007ApJ...664..915B https://ui.adsabs.harvard.edu/abs/2006ApJ...640..360B https://ui.adsabs.harvard.edu/abs/1999ApJ...522L..73B https://ui.adsabs.harvard.edu/abs/1997ApJ...483..320B
- Described in:
- https://ui.adsabs.harvard.edu/abs/1999ApJ...510..759B
- Bibcode:
- 2018ascl.soft09009B
Preferred citation method:
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