An ultraviolet spectral study of fullerene-rich planetary nebulae
Several planetary nebulae (PNe) have been found to contain both polycyclic aromatic hydrocarbon (PAH-like) species and fullerenes (C 60) distinguished by their mid-infrared emission. Previous laboratory and astronomical studies suggest that the formation of both species could be related to the decomposition, by photochemical processing, of
Gómez-Muñoz, M. A. et al.
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2024