Nucleosynthesis Predictions for Intermediate-Mass Asymptotic Giant Branch Stars: Comparison to Observations of Type I Planetary Nebulae
Type I planetary nebulae (PNe) have high He/H and N/O ratios and are thought to be descendants of stars with initial masses of 3-8 M ⊙. These characteristics indicate that the progenitor stars experienced proton-capture nucleosynthesis at the base of th
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|Source:||Astrophysical Journal, The|
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