Comparison of a calculated spectrum of C60H60 with the unidentified astronomical infrared emission features
- 1 August 1991
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 352 (6334) , 412-414
- https://doi.org/10.1038/352412a0
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Hydrocarbon emission features in the IR spectra of warm supergiantsThe Astrophysical Journal, 1990
- The Infrared Interstellar Emission FeaturesPublished by Springer Nature ,1990
- The emission structure between 11 and 13 µm across the Orion ionization frontMonthly Notices of the Royal Astronomical Society, 1989
- Observations of HII Regions and Planetary Nebulae: The Infrared Emission BandsPublished by Springer Nature ,1989
- The Infrared Emission Features and Polycyclic Aromatic HydrocarbonsPublished by Springer Nature ,1989
- The infrared emission bands. I - Correlation studies and the dependence on C/O ratioThe Astrophysical Journal, 1986
- C60: BuckminsterfullereneNature, 1985
- Observations of NGC 7027 from 5.2 to 7.5 microns - The detection of NI II and additional dust featuresThe Astrophysical Journal, 1983
- The 4 to 8 micron spectrum of NGC 7027The Astrophysical Journal, 1977
- 8-13 micron spectra of NGC 7027, BD +30 3639 and NGC 6572.The Astrophysical Journal, 1973