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[ascl:1110.001] analytic_infall: A Molecular Line Infall Fitting Program

This code contains several simple radiative transfer models used for fitting the blue-asymmetric spectral line signature often found in infalling molecular cloud cores. It attempts to provide a direct measure of several physical parameters of the infalling core, including infall velocity, excitation temperature, and line of site optical depth. The code includes 6 radiative transfer models, however the conclusion of the associated paper is that the 5 parameter "hill" model (hill5) is most likely the best match to the physical excitation conditions of real infalling Bonnor-Ebert type clouds.

Code site:
https://bitbucket.org/devries/analytic_infall/wiki/Home
Appears in:
http://adsabs.harvard.edu/abs/2005ApJ...620..800D
Bibcode:
2011ascl.soft10001D

ascl:1110.001
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