Shaping of Planetary Nebulae by Exoplanets
(1) Background: We investigate the hypothesis that exoplanet engulfment can help explain the observed non-spherical planetary nebula population, as a complementary shaping mechanism to the binary hypothesis. The aim is to investigate the extent to which massive planets can explain the population of...
Main Authors: | Nicola Keaveney, Laura Boyle, Matt Redman |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2020-05-01
|
Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/8/2/41 |
Similar Items
-
Planetary nebulae : observations and theory/
by: Planetary Nebulae Symposium (1977, et al.
Published: (1978) -
Whither or Wither the Sulfur Anomaly in Planetary Nebulae?
by: Shuyu Tan, et al.
Published: (2024-01-01) -
The Formation of Fullerenes in Planetary Nebulae
by: Jan Cami, et al.
Published: (2018-09-01) -
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) -
AGBs, Post-AGBs and the Shaping of Planetary Nebulae
by: Eric Lagadec
Published: (2018-09-01)