Cylindrical Planetary Nebulae. I. Flow from an Irradiated Ring
Many bipolar nebulae with a pronounced cylindrical shape, such as Henize 3-401, show no indication whatsoever of interaction between a disk and a stellar wind, or a jet on the nebular axis. I propose that the disk that is observed at the base of the bipolar is itself the source of the outflow. In pa...
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| Format: | Article |
| Language: | English |
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MDPI AG
2022-03-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/10/2/53 |