Commit 033199c9e73a3a90bb439b2f67098d8fa93c63bf

Authored by Jalabert
1 parent 7d6eff78
Exists in master

Update Readme

Showing 1 changed file with 2 additions and 2 deletions   Show diff stats
@@ -33,7 +33,7 @@ For the interstellar medium, the parameters star_radius, parsec and RF_list @@ -33,7 +33,7 @@ For the interstellar medium, the parameters star_radius, parsec and RF_list
33 are no longer important; 33 are no longer important;
34 the part of the program executed will be independent of them 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 *Description* : 37 *Description* :
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. 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 @@ -56,7 +56,7 @@ This main program computes the photoelectric heating rate and efficiency by PAHs
56 Interstellar Radiation Field; if true, then the filename is a file for ISRF 56 Interstellar Radiation Field; if true, then the filename is a file for ISRF
57 if false, the radiation field of a star is studied (default: False) 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 ## Useful files 62 ## Useful files