Shock fronts produced by stellar winds in the interstellar gas

Details Shock fronts produced by stellar winds in the interstellar gas Shock fronts produced by stellar winds in the interstellar gas

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...116..348h&link_type=abstract

Astronomy and Astrophysics, vol. 116, no. 2, Dec. 1982, p. 348-350.

Astronomy and Astrophysics

Astrophysics

14

Interstellar Gas, Shock Fronts, Shock Wave Profiles, Stellar Winds, Differential Equations, Mean Free Path, Stellar Mass Ejection

Scientific paper

A simple method is described for determining the geometrical properties of the shock front which is produced by a stellar wind interacting with an interstellar medium of large relative velocity. The differential equations for this problem are solved numerically. Except for a trivial scaling factor, the resulting geometrical form of the front is the same for all combinations of stellar winds and interstellar properties.

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