Hydrodynamical models of clumping beyond 50 stellar radii

M. C. Runacres

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arXiv · 0711.1939

Hydrodynamical models of clumping beyond 50 stellar radii

M. C. Runacres

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Abstract

We present one-dimensional, time-dependent models of the clumps generated by the line-deshadowing instability. In order to follow the clumps out to distances of more than 1000 stellar radii, we use an efficient moving-box technique. We show that, within the approximations, the wind can remain clumped well into the formation region of the radio continuum.

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M. C. Runacres. 2007-11-13. Hydrodynamical models of clumping beyond 50 stellar radii. https://arxiv.org/abs/0711.1939

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