First results of the modelling of the two-component radiatively driven
stellar wind were published in the poster at conforence in Tartu
(text,figures). Brief
article from proceedings is available too.
During my diploma work I computed K giant
model atmospheres. For this purpose I used Hubeny's program TLUSTY and
Kurucz's progam ATLAS. I have modified program SYNSPEC slighly
(inclusion of atoms with Z in the range 30 < Z <= 90, inclusion of Plez's
input files), you can download it from this
ftp directory. I determined atmosphere parameters of some K-giants.
Some information about this topic you can find in papers, which I wrote
mostly with Dr. V. Stefl:
you can download poster from The Conference
of Czech and Slovak Astronomers, Brno, 1997 (the
English or the
Czech version),
here is available my diploma work (only in Czech). I discussed model atmospheres used for K-giants and
determined basic parameters of four K-giants.
My work was briefly described in article written
for Brno Supercomputing Center (Czech
or English version).
