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README.md
... | ... | @@ -33,7 +33,7 @@ For the interstellar medium, the parameters star_radius, parsec and RF_list |
33 | 33 | are no longer important; |
34 | 34 | the part of the program executed will be independent of them |
35 | 35 | |
36 | -**three_levels_model.py** : | |
36 | +**four_levels_model.py** : | |
37 | 37 | *Description* : |
38 | 38 | This main program computes the photoelectric heating rate and efficiency by PAHs. The expressions used are based on the model with 4 charge states of the molecule, going from the anion molecule (charge state Z=-1) to the dication (charge state Z=2) by ionization. |
39 | 39 | |
... | ... | @@ -56,7 +56,7 @@ This main program computes the photoelectric heating rate and efficiency by PAHs |
56 | 56 | Interstellar Radiation Field; if true, then the filename is a file for ISRF |
57 | 57 | if false, the radiation field of a star is studied (default: False) |
58 | 58 | |
59 | - This program uses radiations_fields.py. | |
59 | +This program uses radiations_fields.py. | |
60 | 60 | |
61 | 61 | |
62 | 62 | ## Useful files | ... | ... |