Hydrodynamical models of clumping beyond 50 stellar radii

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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.
International Workshop on clumping in Hot-Star Winds, June 2007, Potsdam, Germany. (3 pages, 2 figures)

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/142018

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0711.1939
 http://arxiv.org/abs/0711.1939

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arXiv