Will include atlases and computed spectra
Directory [STARS] logical name STARS
Subdirectory [STARS.logical name]
This is just my list of directories with star names.
Not all of these will end up on the web.
Others will be added.
109995
51PEG
ALPHACEN:
ALTAIR
ARCTURUS:
ASTAR:
BD75325
BETAPIC
BETELGEUSE:
BSTAR
CANOPUS
CAPELLA
CHILUPI
DELTASCO
GL411:
HD189733:
HD209458:
HD72660
HR152
K0V:
LAMBDABOO
M5V:
MUCAS
MUGEM
POPIIMDWARF:
PROCYON:
SAKURAI
SIRIUS:
SPICA
SUN:
TAUSCO
VEGA:
XO-1 = GSC 02041-01657:
I have started copying the test spectrum calculations
that are extant to the web directory. These spectra require
considerable improvement before they can be considered
realistic. They were calculated either at resolving power
of 500000 or 2000000 in Doppler space so that a shift in
point number is a Doppler shift. The wavelengths were
generated from the expression
WL=WLFIRST*(1.D0+1.D0/RESOLUTION)**(IWL-1).
Some of the spectra have been instrumentally broadened with a
gaussian to smaller resolving powers at the same wavelengths
using program BROADEN. The broadened spectra were then resampled
at the center of an odd number of points using program RESAMPLE.
The new points are uniformly spaced in doppler space.
The spectra are presented in wavelength (nm), Hlambda
(ergs/s/cm**2/ster/nm), and continuum Hlambda (ergs/s/cm**2/
ster/nm) triplets. The model atmosphere and a sample .COM
file are also given. The programs are changing rapidly, as
are the line data, so the same spectrum computed today might
be different, hopefully improved. Also the model atmosphere
probably does not have the correct parameters for the star.
In the detailed study of each star it is necessary to compute
many models and many spectra, varying the parameters.