C₆₀ in Reflection Nebulae

October 2010 • 2010ApJ...722L..54S

Authors • Sellgren, Kris • Werner, Michael W. • Ingalls, James G. • Smith, J. D. T. • Carleton, T. M. • Joblin, Christine

Abstract • The fullerene C₆₀ has four infrared-active vibrational transitions at 7.0, 8.5, 17.4, and 18.9 μm. We have previously observed emission features at 17.4 and 18.9 μm in the reflection nebula NGC 7023 and demonstrated spatial correlations suggestive of a common origin. We now confirm our earlier identification of these features with C₆₀ by detecting a third emission feature at 7.04 ± 0.05 μm in NGC 7023. We also report the detection of these three C₆₀ features in the reflection nebula NGC 2023. Our spectroscopic mapping of NGC 7023 shows that the 18.9 μm C₆₀ feature peaks on the central star and that the 16.4 μm emission feature due to polycyclic aromatic hydrocarbons peaks between the star and a nearby photodissociation front. The observed features in NGC 7023 are consistent with emission from UV-excited gas-phase C₆₀. We find that 0.1%-0.6% of interstellar carbon is in C₆₀; this abundance is consistent with those from previous upper limits and possible fullerene detections in the interstellar medium (ISM). This is the first firm detection of neutral C₆₀ in the ISM.

Links

• SIMBAD http://simbad.u-strasbg.fr/simbo.pl?bibcode=2010ApJ...722L..54S
• PDF https://iopscience.iop.org/article/10.1088/2041-8205/722/1/L54/pdf
• PDF https://stacks.iop.org/2041-8205/722/L54/pdf
• PREPRINT http://arxiv.org/abs/1009.0539
• DATA https://irsa.ipac.caltech.edu/bibdata/2010/S/2010ApJ...722L..54S.html
• ELECTR https://doi.org/10.1088%2F2041-8205%2F722%2F1%2FL54