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| Simple Stellar Atmospheres |
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Contact: F.X.Timmes
my one page vitae,
full vitae,
research statement, and
teaching statement.
The tool public_atmos.tbz implements a simple stellar atmosphere model. It assumes a one-dimensional slab in hydrostatic and local thermodynamic equilibrium with gray rosseland mean opacities. Still, it can be useful as a quick diagnostic of a stellar atmosphere, or for checking the effects of a more elaborate piece of local physics (e.g., ionization, such as the figure on the right).
1 M☉ temperature structure |
1 M☉ ionization structure |