A computer program for calculating the structure of magnetohydrodynamical shocks in interstellar clouds

Details A computer program for calculating the structure of magnetohydrodynamical shocks in interstellar clouds A computer program for calculating the structure of magnetohydrodynamical shocks in interstellar clouds

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cophc..58..169h&link_type=abstract

Computer Physics Communications, Volume 58, Issue 1-2, p. 169-179.

Physics

16

Scientific paper

The program solves for the stationary-state profile of a shock propagating in the interstellar medium under the influence of a magnetic field. The number densities of a given set of atomic and molecular species are computed point by point through the shock. Heavy molecules of the polycyclic aromatic hydrocarbon type, for example, may be included amongst the molecular species.

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