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[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
Appears in:
http://adsabs.harvard.edu/abs/1997ApJ...483..320B http://adsabs.harvard.edu/abs/1999ApJ...510..759B http://adsabs.harvard.edu/abs/1999ApJ...522L..73B http://adsabs.harvard.edu/abs/2006ApJ...640..360B http://adsabs.harvard.edu/abs/2007ApJ...664..915B
Bibcode:
2018ascl.soft09009B

Views: 122

ascl:1809.009
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