Abstract
We report on the detection of a molecular band centered at $98 m ($102 cm À1), observed with the Infrared Space Observatory in the young planetary nebula NGC 7027. The band structure and intensity cannot be reproduced by atomic fine-structure lines, recombination lines, or the rotational emission of abundant molecules. We discuss the possible contribution of the low-energy bending modes of pure carbon chains to the unidentified far-IR bands observed in C-rich evolved objects. In particular, we speculate that the band emission could arise from the 9 and 7 bending modes of C 6 and C 5 , for which wavenumbers of 90 AE 50 and 107 AE 5 cm À1 have been estimated from photoelectron spectroscopy.
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CITATION STYLE
Goicoechea, J. R., Cernicharo, J., Masso, H., & Senent, M. L. (2004). A New Unidentified Far‐Infrared Band in NGC 7027. The Astrophysical Journal, 609(1), 225–230. https://doi.org/10.1086/421061
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