Programas
"Stellar Interiors," 2nd ed., by Hansen, Kawaler, & Trimble
Copyright 2004, Springer-Verlag, NY
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FORTRAN computer programs and
demonstration modules relevant to stellar structure and evolution. They come
from several sources, including colleagues and friends in astronomy and
astrophysics, and some are due to the authors of the text. We have made
every attempt to make them user-friendly, although some modules will only run
on Windows based PCs.
There are eight
sub-directories, listed below
with a brief description of their contents. Note that each of these directories
contain their own readme files in which you will find many more details.
The sub-directories are, in alphabetical order,
ATMOS: a Windows PC executable file to construct gray
atmospheres (by Odell & Pesnell). The output is graphical.
BZAMS: three versions of a FORTRAN code to compute
main sequence models (plus Windows PC executable files).
The versions differ only in what equations of state and
opacities are used. A code for analyzing pulsations is
also included.
EVOLUTION: contains Windows PC executable files to make main sequence
models and evolve them (for 1 and 10 solar masses). The output
is graphical (by Odell & Pesnell).
MISC: contains FORTRAN programs to compute simple equations of
state and Cox-Stewart opacities. Windows PC executable files
are also included.
PACZYNSKI: contains versions of the "Paczynski" codes (in FORTRAN plus
Windows PC executables) to evolve hydrogen burning models.
StellarEvolnDemo: a tutorial on stellar evolution and nucleosynthesis
(by Lattanzio and colleagues). It is in HTML.
WD: a FORTRAN code (plus a Windows PC executable file) to make
zero-temperature electron degenerate white dwarfs.
ZamsPuls: two FORTRAN codes (plus Windows PC executable files)
to make main sequence models and analyze them for adiabatic
pulsations.
