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- W1640563734 abstract "The formation of ring nebulae and their shapes is studied by numerical simulations. The old problem of the origin of the nebular shape is addressed. Two proposed mechanisms are discussed: stellar rotation and stellar magnetic fields, or a combination of both. Two and three-dimensional hydrodynamical and magneto-hydrodynamical simulations indicate that these processes are equally efficient in driving elliptical nebulae such as those surrounding Wolf-Rayet stars, like NGC 6888 around WR136. However, bipolar nebulae are better reproduced by rotation." @default.
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- W1640563734 date "1999-01-01" @default.
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- W1640563734 title "Hydrodynamics of ring nebulae: magnetic vs. non-magnetic hydro-models" @default.
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- W1640563734 doi "https://doi.org/10.1017/s0074180900205597" @default.
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