Theoretical predictions for the cold part of the colliding wind interaction zone

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dc.creatorFolini, D.
dc.creatorWalder, R.
dc.date2000-12-06
dc.date.accessioned2026-07-07T01:56:54Z
dc.date.available2026-07-07T01:56:54Z
dc.descriptionWe present 2D and 3D hydrodynamical simulations of the colliding wind interaction zone in WR+O binaries. It is shown that 3D effects can basically explain certain observed, orbit dependent flux variations. Possible connections between the interior structure of the interaction zone and dust formation are outlined and its stability is re-investigated.
dc.description6 pages, 2 figures, to appear in PASP conference series, proceedings of the workshop 'Interacting Winds from Massive Stars'
dc.identifierhttps://arxiv.org/abs/astro-ph/0012132
dc.identifierhttp://arxiv.org/abs/astro-ph/0012132
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2171
dc.subjectAstrophysics
dc.titleTheoretical predictions for the cold part of the colliding wind interaction zone
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