Tracing the Evolution of the Emission Properties of Carbon-Rich AGB, Post-AGB, and PN Sources

Understanding the transition from the Asymptotic Giant Branch (AGB) to the Planetary Nebula (PN) phase is crucial for advancing our knowledge of galaxy evolution and the chemical enrichment of the universe. In this manuscript, we analyze 137 carbon-rich, evolved low- and intermediate-mass stars (LIM...

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Bibliographic Details
Main Authors: Silvia Tosi, Ester Marini
Format: Article
Language:English
Published: MDPI AG 2025-01-01
Series:Astronomy
Subjects:
Online Access:https://www.mdpi.com/2674-0346/4/1/2
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