The propagation of periodical shock waves and the large gradient velocity structures caused by stellar pulsation.

Details The propagation of periodical shock waves and the large gradient velocity structures caused by stellar pulsation. The propagation of periodical shock waves and the large gradient velocity structures caused by stellar pulsation.

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ppmto...9..104h&link_type=abstract

Publ. Purple Mt. Obs., Vol. 9, No. 2, p. 104 - 115

Other

Stellar Models: Shock Waves, Stellar Models: Pulsations, Stellar Models: Mira Stars

Scientific paper

The method of calculating periodical shock waves in Eulerian coordinates is presented. Propagating process of shock waves caused by stellar pulsation in the outer layers of a typical Mira Variable is described. A shock wave propagates outward once period. In the adiabatic case a steady mass loss far from star is produced by shock wave. In the isothermal case the energy of shock wave is dissipated within the range of several piston radii.

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