Modeling the cometary structure of the planetary nebula HFG1 based on the evolution of its binary central star V664 Cas

Monthly Notices of the Royal Astronomical Society(2016)

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摘要
HFG1 is the first well-observed planetary nebula (PN) which reveals a cometary-like structure. Its main morphological features consist of a bow-shaped shell, which surrounds the central star, accompanied by a long collimated tail. In this study, we perform two-dimensional hydrodynamic simulations modelling the formation of HFG1 from the interaction of the local ambient medium with the mass outflow...
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hydrodynamics,stars: AGB and post-AGB,stars: individual: V664 Cas,subdwarfs,planetary nebulae: individual: HFG1
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