Asphaltenes as model compounds of the UIBs/AIBs detected in various astrophysical objects. Part 3: Petroleum asphaltenes high energy radiation processed

Bibcode
2022FNCN...30..923G
DOI
10.1080/1536383X.2022.2040487
García-Hernández, Domingo Aníbal; Manchado, Arturo; Cataldo, Franco
Bibliographical reference

Fullerene Nanotubes and Carbon Nanostructures

Advertised on:
9
2022
Number of authors
3
IAC number of authors
2
Citations
1
Refereed citations
1
Related projects
Project Image
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
Domingo Aníbal
García Hernández
In progress
Type
Refereed
Exoplanetary Systems & Solar System (SEYSS)
Stellar & Interstellar Physics (FEEI)
The Milky Way and the Local Group (MWLG)

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