On the Detectability of Post-common-envelope Binary Central Stars of Planetary Nebulae
Common envelope evolution is widely accepted as the principal shaping agent in the formation of aspherical planetary nebulae. However, only some 20% of planetary nebulae are found to host post-common-envelope binary central stars. To probe the detectability of post-common-envelope binary central stars, and their potential to evade detection, we
Hume, George et al.
Fecha de publicación:
3
2022