作者: S. Mohamed , R. Booth , Ph. Podsiadlowski , S. Ramstedt , W. Vlemmings
DOI: 10.1051/EAS/1571015
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摘要: Symbiotic binaries consist of a cool, mass-losing giant and an accreting, compact companion. We present 3D Smoothed Particle Hydrodynamics (SPH) models two such interacting binaries, RS Oph Mira AB. is also recurrent nova system, thus we model multiple quiescent mass transfer-nova outburst cycles. The resulting circumstellar structures both systems are highly complex with the formation spirals, arcs, shells, equatorial bipolar outflows. compare to recent observations discuss implications our results for related systems, e.g., nebulae jets, chemically peculiar stars, progenitors Type Ia supernovae.