Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...464l.191m&link_type=abstract
Astrophysical Journal Letters v.464, p.L191
Astronomy and Astrophysics
Astronomy
43
Ism: Dust, Extinction, Ultraviolet: Ism, Methods: Laboratory
Scientific paper
The results of an experiment aimed at simulating the UV processing of hydrogenated amorphous carbon grains that occurs in the interstellar medium are presented. UV exposure of these grains induces significant changes in the UV-visible spectrum and, in particular, activates a resonance at 215 +/- 2 nm, very close to the position of the interstellar extinction bump. This is the first reported laboratory observation of the activation of a UV resonance in hydrogenated carbon grains irradiated by UV photons. The spectral variations depend on the UV dose deposited in the samples; as the dose increases, the band becomes more intense while its peak position remains stable. We attribute the band to pi -- pi * electronic transitions in sp2 ringed clusters that form the grains and interpret the spectral variations in terms of structural changes of the grains. This interpretation is confirmed by the behavior of the optical gap, which indicates an increase of the sp2 clustering degree as a function of the grain processing. The results of the present experiment suggest that it is unlikely that hydrogenated amorphous carbon grains can be transformed into pure graphite grains by UV processing in a typical diffuse-cloud timescale. The possibility that the interstellar bump is due to pi -- pi * transitions in graphitic clusters that form small carbon grains is analyzed. This hypothesis requires a definite internal structure for the bump carrier. A process able to determine the grain structure is briefly discussed.
Bussoletti Ezio
Colangeli Luigi
Mennella Vito
Palumbo Pasquale
Rotundi Alessandra
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