[Li@C60]PF6: Infrared spectra from 90K to 523K; Determination of the molar extinction coefficients and integrated molar absorptivity

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

Fullerene Nanotube]s and Carbon Nanostructures

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6
2020
Number of authors
3
IAC number of authors
2
Citations
4
Refereed citations
4
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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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