A hydrodynamic code for the treatment of late-type stellar wind flows based on the method of characteristics

Details A hydrodynamic code for the treatment of late-type stellar wind flows based on the method of characteristics A hydrodynamic code for the treatment of late-type stellar wind flows based on the method of characteristics

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...193..119c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 193, no. 1-2, March 1988, p. 119-124.

Astronomy and Astrophysics

Astrophysics

28

Hydrodynamic Equations, Late Stars, Method Of Characteristics, Stellar Atmospheres, Stellar Winds, Boundary Value Problems, Shock Wave Propagation, Solar Corona, Stellar Mass Ejection

Scientific paper

The authors describe a time-dependent eulerian hydrodynamic code based on the method of characteristics which allows the computation of radiating stellar wind flows in tube-like structures on late-type stars. The treatment of boundaries under sub- and supersonic conditions is discussed as is the introduction of shock waves into the atmosphere. Ionization is taken into account. For test and application the authors study the behaviour to approach limiting shock strength.

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