Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...297..835p&link_type=abstract
Astronomy and Astrophysics, v.297, p.835
Astronomy and Astrophysics
Astrophysics
14
Stars: Mass-Loss, Shock Waves, Hydrodynamics, Sun: Solar Wind, Ism: Kinematics And Dynamics
Scientific paper
A gasdynamic interaction is considered between a non-stationary periodically changing stellar wind and the interstellar medium. Substantial nonsteady elements of the flow structure are detected, characterized by the periodical appearance of shock waves arising due to the compression disturbances transition through the internal shock wave. Numerical calculations are performed for parameters modeling the 11-year solar activity.
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