Hydrodynamics of stellar wind of hot stars

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Project Identification
GP205/03/D020
Project Period
9/2003 - 8/2006
Investor / Pogramme / Project type
Czech Science Foundation
MU Faculty or unit
Faculty of Science
Keywords
Astronomy and celestial mechanics, astrophysics

In the cooperation with the supervisor of Ph.D. study RNDr. Jioí Kubát,
CSc., the proposer of this project successfully developed models
describing multicomponent radiatively driven stellar wind of hot stars.
However, this models are computed usingsimpli fied calculation of
radiative force and thermal balance. The purpose of submitted project is
to extend mentioned multicomponent models in order to obtain
sell-consistent models of hot star winds. The description of stellar winds
with relatively lowdensit y will be improved. Obtained models will be
directly compared with observed quantities. In this sense the submitted
project extends the basic project GA ČR 205/ 02/445 "Physics of hot stars
and stellar systems with hot components.

Publications

Total number of publications: 18


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