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Nucleosynthesis Predictions for Intermediate-Mass Asymptotic Giant Branch Stars: Comparison to Observations of Type I Planetary Nebulae

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Karakas, Amanda
van Raai, M. A.
Lugaro, Maria Anna
Sterling, Nicholas
Dinerstein, Harriet

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IOP Publishing

Abstract

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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Astrophysical Journal, The

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Restricted until

2037-12-31