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Gasdynamics of Detached Shells Around Carbon Stars With Variable Mass Loss

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Abstract

Gasdynamic features of detached shells around carbon stars with variable mass loss rate are investigated in detail numerically. It is shown that a shell is unstable and also, 2D perturbations are less developed that 3D ones. The structure of perturbed flows corresponding to different evolution scenarios is compared. The results obtained seem to be promising for interpretation of observations, in particular, the recently obtained detailed data of TT Cyg.

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Authors and Affiliations

  1. Institute for problems in mechanics, Moscow, Russia

    A.V. Myasnikov & N.A. Belov

  2. Uppsala Astronomical Observatory, Uppsala, Sweden

    B. Gustafsson & K. Eriksson

Authors
  1. A.V. Myasnikov
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  2. N.A. Belov
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  3. B. Gustafsson
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  4. K. Eriksson
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Myasnikov, A., Belov, N., Gustafsson, B. et al. Gasdynamics of Detached Shells Around Carbon Stars With Variable Mass Loss. Astrophysics and Space Science 274, 231–241 (2000). https://doi.org/10.1023/A:1026520628041

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