Binary Interactions, High-Speed Outflows and Dusty Disks during the AGB-To-PN Transition
It is widely believed that the dramatic transformation of the spherical outflows of AGB stars into the extreme aspherical geometries seen during the planetary nebula (PN) phase is linked to binarity and driven by the associated production of fast jets and central disks/torii. The key to understandin...
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| Format: | Article |
| Language: | English |
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MDPI AG
2018-09-01
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| Series: | Galaxies |
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| Online Access: | http://www.mdpi.com/2075-4434/6/4/102 |