3D models of the circumstellar environments of evolved stars: Formation of multiple spiral structures
We present 3D hydrodynamic models of the interaction between the outflows of evolved, pulsating, Asymptotic Giant Branch (AGB) stars and nearby (<3 stellar radii) substellar companions (Mcomp 40MJ). Our models show that due to resonances between the orbital period of the companion and the pulsati...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Oxford University Press
2022
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| Subjects: | |
| Online Access: | View Fulltext in Publisher |