On the formation of molecules and solid-state compounds from the AGB to the PN phases
During the asymptoyic giant branch (AGB) phase, different elements are dredge- up to the stellar surface depending on progenitor mass and metallicity. When the mass loss increases at the end of the AGB, a circumstellar dust shell is formed, where different (C-rich or O-rich) molecules and solid-state compounds are formed. These are further
García-Hernández, D. A. et al.
Fecha de publicación:
7
2016