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...
Main Author: | Vincent Icke |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2022-03-01
|
Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/10/2/53 |
Similar Items
-
Millimetre Observations of Maser-Emitting Planetary Nebulae
by: Lucero Uscanga, et al.
Published: (2022-03-01) -
Neutron-Capture Element Abundances in Planetary Nebulae
by: N. C. Sterling
Published: (2020-06-01) -
Stars and nebulas/
by: 406227 Kaufmann, William J.
Published: (1978) -
Numerical Models of Planetary Nebulae with Different Episodes of Mass Ejection: The Particular Case of HuBi 1
by: Ary Rodríguez-González, et al.
Published: (2023-01-01) -
When the Stars Align: A 5σ Concordance of Planetary Nebulae Major Axes in the Center of Our Galaxy
by: Shuyu Tan, et al.
Published: (2023-01-01)