Hydrodynamical models of clumping beyond 50 stellar radii

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dc.creatorRunacres, M. C.
dc.date2007-11-13
dc.date.accessioned2026-07-07T08:42:36Z
dc.date.available2026-07-07T08:42:36Z
dc.descriptionWe 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.
dc.descriptionInternational Workshop on clumping in Hot-Star Winds, June 2007, Potsdam, Germany. (3 pages, 2 figures)
dc.identifierhttps://arxiv.org/abs/0711.1939
dc.identifierhttp://arxiv.org/abs/0711.1939
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142018
dc.subjectAstrophysics
dc.titleHydrodynamical models of clumping beyond 50 stellar radii
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