These are the most frequently used words in this book.
2000
abundance
agb
al
apj
atmosphere
between
binary
carbon
case
chapter
chemical
co
core
cse
density
different
distribution
due
during
dust
effects
emission
energy
envelope
et
evolution
few
field
fig
figure
first
form
formation
found
galaxy
gas
giant
given
grains
high
however
important
increase
large
line
loss
low
luminosity
maser
mass
may
mira
models
molecular
molecules
number
objects
observations
observed
period
phase
point
pressure
processes
pulsation
pulse
radiation
radiative
radius
rate
ratio
region
results
scale
section
see
shell
should
shows
since
source
spectral
stars
stellar
structure
study
surface
systems
temperature
thermal
thus
time
two
used
value
variables
velocity
wavelengths
wind