For over 20 years the infrared spectra of many astronomical objects have been interpreted as flat two-dimensional polycyclic aromatic hydrocarbons (PAHs) that are also thought to be the source of organic matter on our own planet. More recently the detection of molecules such as fullerenes – molecules composed entirely of carbon, including the spherical C60 – has revealed a more complicated picture of carbon in space. The links between these different molecules have been rather unclear but new research from Héctor Alvaro Galué at VU University of Amsterdam, in the Netherlands, has taken a fresh approach to this long-standing puzzle.
Energetic particles in interstellar space induce strain and re-hybridisation within flat carbon structures. Background image: © NASA, ESA, M Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team
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Decoding the infrared signatures of pyramidal carbons in graphenic molecular nanostructures of interstellar origin
Hector Alvaro Galue
Chem. Sci., 2014, Accepted Manuscript, DOI: 10.1039/C4SC00890A, Edge Article
