Search For C_60

Details Search For C_60 Search For C_60

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40276s&link_type=abstract

Spitzer Proposal ID #40276

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Scientific paper

We propose to follow up on our recent Spitzer IRS-LL2 detection of emission at 17.4 and 18.9 um in the reflection nebulae NGC 2023 and NGC 7023. These wavelengths coincide with two of the four infrared lines of buckminsterfullerene, or C_60. Our goal is to obtain IRS-SL spectra to confirm this identification by searching for the two other infrared C_60 lines, at 7.1 and 8.5 um. We will also obtain IRS-SH spectra to measure the widths of the 17.4 and 18.9 um lines, which depend on temperature for C_60.

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