Understanding Galactic planetary nebulae with precise/reliable nebular abundances
We compare recent precise/reliable nebular abundances - as derived from high-quality optical spectra and the most recent ICFs - in a sample of Galactic planetary nebulae (PNe) with nucleosynthesis predictions (HeCNOCl) from asymptotic giant branch (AGB) ATON models in the metallicity range Z ⊙/4 Z 2Z ⊙. According to the infrared dust features
García-Hernández, D. A. et al.
Advertised on:
10
2017