Asphaltenes as model compounds of the UIBs/AIBs detected in various astrophysical objects. Part 1 – Petroleum asphaltenes carbonization

Cataldo, Franco; García-Hernández, D. Aníbal; Manchado, Arturo
Bibliographical reference

Fullerene Nanotubes and Carbon Nanostructures

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5
2022
Number of authors
3
IAC number of authors
2
Citations
4
Refereed citations
4
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Nucleosynthesis and molecular processes in the late stages of Stellar Evolution
Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch (AGB) - just before they form planetary nebulae (PNe) - where they experience complex nucleosynthetic and molecular processes. AGB stars are important contributors to the enrichment of the
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