Abstract
The program calculates model stellar atmospheres, assuming plane-parallel, horizontally homogeneous atmosphere in radiative and hydrostatic equilibrium, and allowing for departures from local thermodynamic equilibrium (LTE) for a set of occupation numbers of selected atomic and ionic energy levels. The program is very flexible as to the choice of chemical.
Original language | English (US) |
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Pages (from-to) | 103-132 |
Number of pages | 30 |
Journal | Computer Physics Communications |
Volume | 52 |
Issue number | 1 |
DOIs | |
State | Published - Dec 1988 |
Externally published | Yes |
ASJC Scopus subject areas
- Hardware and Architecture
- Physics and Astronomy(all)