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- W94881859 abstract "The pinwheel nebulae observed in some WC-binaries essentially mirror a transport phenomenon. We show the importance of the central wind collision zone in setting the ‘initial conditions’ for this transport. In order to understand some of the newly observed features, we postulate that standard theory of colliding flows must be extended by considering radiative breaking, heat-conduction, and the clumped character of the winds. We suggest that clumped winds can be modeled by highly compressible turbulence and outline some consequences for the physics of the wind collision zone. With regard to dust production we argue that the system center is the only location where dust nucleation can happen." @default.
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- W94881859 date "2003-01-01" @default.
- W94881859 modified "2023-09-26" @default.
- W94881859 title "3D-hydrodynamics of colliding winds in massive binaries" @default.
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- W94881859 doi "https://doi.org/10.1017/s0074180900211741" @default.
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