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.gitignore.txt
README.md
README.rtf deleted
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2 | -{\fonttbl\f0\fswiss\fcharset0 Helvetica;} | |
3 | -{\colortbl;\red255\green255\blue255;} | |
4 | -{\*\expandedcolortbl;;} | |
5 | -\paperw11900\paperh16840\margl1440\margr1440\vieww14300\viewh7720\viewkind0 | |
6 | -\pard\tx566\tx1133\tx1700\tx2267\tx2834\tx3401\tx3968\tx4535\tx5102\tx5669\tx6236\tx6803\pardirnatural\partightenfactor0 | |
7 | - | |
8 | -\f0\fs24 \cf0 Welcome in the directory concerning the study of the influence of PAH on the gas heating by photoelectric effect.\ | |
9 | -\ | |
10 | -Description of the files:\ | |
11 | - - coupes_fits.py: library defining a function allowing to cut a map between 2 points. Used in the code \'ab\'a0photoelectric_heating_model_ngc7023nw.py\'a0\'bb to obtain the cuts along 3 lines of sight with HD200775 as a reference.\ | |
12 | - \ | |
13 | - -fov_data_NGC7023_H2.py : code extracting the useful information from all the maps stored in \'abthe \'ab\'a0data\'a0\'bb directory. Read its documentation to know how it produces a dictionary containing the information on the common field of view between IRS and PACS observations.\ | |
14 | -\ | |
15 | - - NGC7023_map_analysis_f0evsg.py : code in which some computation and plots are done, in particular to compute the PE heating efficiency, ionization fraction\'85\ | |
16 | -\ | |
17 | - - \'ab\'a0photoelectric_heating_model_ngc7023nw.py\'a0\'bb : Mol\'e9cular model of the photoelectric heating on PAH, using data of laboratory experiments and quantum chemistry computations. \ | |
18 | -All the directories here are related to this code, see below.\ | |
19 | -\ | |
20 | - - \'ab\'a0 photoionization_lib.py\'a0\'bb : library of functions used is the code \'ab\'a0photoelectric_heating_model_ngc7023nw.py\'a0\'bb.\ | |
21 | -\ | |
22 | - - reproj_lib.py : library of the functions used in the code \'abfov_data_NGC7023_H2.py\'a0\'bb \'a0to produce maps downgraded to the coordinate frame and spatial resolution of the [Cii] 158mu PACS map (11\'92\'92).\ | |
23 | -\ | |
24 | -Look at the \'ab\'a0reproj_lib.py\'a0\'bb description for the methodology used to produce the maps.\ | |
25 | - \ | |
26 | -\ | |
27 | -Description of the directories:\ | |
28 | - - \'ab\'a0neutrals\'a0\'bb, \'ab\'a0cations\'a0\'bb and \'ab\'a0dication\'a0\'bb: directories where the photo absorption cross sections are stored (Spectral database of Theoretical PAH, Malocci et al 2007)\ | |
29 | - - images_molecules : png image of the molecules considered (from the database)\ | |
30 | - -yields: now useless in the code of the model (the yields are generated by a function) but contains the photoionization yields of several studies (see titles and descriptions of these files)\ | |
31 | - -extinction_curves : Obvious purpose, from Weingartner and Draine 2001\ | |
32 | - -radiation_fields : contains the radiation fields of Habing (1968), Mathis (1983) and Draine (noted ISRF). They come from the following website: https://home.strw.leidenuniv.nl/~ewine/photo/radiation_fields.html\ | |
33 | -The HD200775_RF.txt is the radiation field of the star HD200775\ | |
34 | -\ | |
35 | - \ | |
36 | -} | |
37 | 0 | \ No newline at end of file |
main_program.py renamed to three_levels_model.py