A linear stability analysis for wind-driven bubbles

Details A linear stability analysis for wind-driven bubbles A linear stability analysis for wind-driven bubbles

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...331..350r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 331, Aug. 1, 1988, p. 350-358.

Astronomy and Astrophysics

Astrophysics

24

Bubbles, Dynamic Stability, Interstellar Gas, Shock Waves, Stellar Winds, Adiabatic Conditions, Perturbation Theory, Shock Fronts

Scientific paper

The authors examine the growth of linear perturbations of adiabatic shells of the shocked interstellar gas surrounding a strong stellar wind. The shells are overstable if the adiabatic index γ ⪉ 1.1, and most overstable for the wavelengths comparable to the thickness of the shell. The shells of the wind-driven bubbles are generally more stable than those of blast waves. The implications of these results are discussed.

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