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33 for( nd=0; nd <
gv.
nBin; nd++ )
56 " gas heating by grain photoionization");
59 " gas heating by thermionic emissions of grains ");
62 "gas cooling by collisions with grains ");
65 " gas heating by collisions with grains ");
68 " total grain heating by all sources, lines, collisions, incident continuum ");
71 " grain heating by incident continuum ");
74 " grain heating due to destruction of Ly alpha ");
77 " grain heating due to collisions with gas ");
80 " grain heating due to diffuse fields, may also have grain emission ");
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