3D stability analysis of colliding winds in a double star system

Details 3D stability analysis of colliding winds in a double star system 3D stability analysis of colliding winds in a double star system

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...271..527d&link_type=abstract

Astronomy and Astrophysics, Vol. 271, p. 527 (1993)

Astronomy and Astrophysics

Astrophysics

5

Colliding Winds, Double Star Systems, Hydrodynamics, Stability Analysis

Scientific paper

We continue the study of the stability of a collision front between two identical winds in a double star system in the limit of isothermal flows, with Mach number M = ∞, by investigating the behaviour of the azimuthal modes. We thus extend a previous work that dealt with the cylindrically symmetrical case. In contrast to the behaviour of the radial and tangential modes, the azimuthal modes are stable against small wavelength perturbations.

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