AGBs, Post-AGBs and the Shaping of Planetary Nebulae
During the last decades, observations, mostly with the Hubble Space Telescope, have revealed that round Planetary Nebulae were the exception rather than rule. A huge variety of features are observed, such as jets, discs, tori, showing that the ejection of material is not due to isotropic radiation p...
Main Author: | Eric Lagadec |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2018-09-01
|
Series: | Galaxies |
Subjects: | |
Online Access: | http://www.mdpi.com/2075-4434/6/3/99 |
Similar Items
-
Millimetre Observations of Maser-Emitting Planetary Nebulae
by: Lucero Uscanga, et al.
Published: (2022-03-01) -
Planets, Planetary Nebulae, and Intermediate Luminosity Optical Transients (ILOTs)
by: Noam Soker
Published: (2018-05-01) -
Observing the signatures of AGB s-process nucleosynthesis in planetary nebulae: An origins story
by: Harriet L. Dinerstein
Published: (2022-12-01) -
Mass Transfer in Two Post-AGB Binaries with Dusty Disks
by: Gorlova N., et al.
Published: (2012-06-01) -
Analysis of Multiple Shell Planetary Nebulae Based on HST/WFPC2 Extended 2D Diagnostic Diagrams
by: Daniela Barría, et al.
Published: (2018-08-01)