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