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

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

2000-12-06

arxiv.org/abs/astro-ph/0012132v1

Astronomy and Astrophysics

Astrophysics

6 pages, 2 figures, to appear in PASP conference series, proceedings of the workshop 'Interacting Winds from Massive Stars'

Scientific paper

We 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.

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