On the theory of the propagation of intense shock waves in inhomogeneous gravitating media. II - Radiative cooling phase

Details On the theory of the propagation of intense shock waves in inhomogeneous gravitating media. II - Radiative cooling phase On the theory of the propagation of intense shock waves in inhomogeneous gravitating media. II - Radiative cooling phase

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...15p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, May-June 1986, p. 15-21. In Russian.

Computer Science

3

Gravitation Theory, Shock Wave Propagation, Stellar Gravitation, Equations Of Motion, Inhomogeneity, Shock Fronts, Stellar Mass

Scientific paper

The effect of the gravitational field of stars on the propagation of intense radiative shock waves is investigated in the infinitely thin layer approximation. The equations of motion for shock waves and their analytical solutions are found. Combining the previously obtained solution for the adiabatic phase with the present one, the complete description of the shock wave propagation is obtained.

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