Abstract

The results of a Caltech Submillimeter Observatory (CSO) search for ll-C3_3H+^+, first detected by Pety et al. (2012) in observations toward the Horsehead photodissociation region (PDR), are presented. A total of 39 sources were observed in the 1 mm window. Evidence of emission from ll-C3_3H+^+ is found in only a single source - the Orion Bar PDR region, which shows a rotational temperature of 178(13) K and a column density of 7(2) x 101110^{11} cm−2^{-2}. In the remaining sources, upper limits of ~1011−1013^{11} - 10^{13} cm−2^{-2} are found. These results are discussed in the context of guiding future observational searches for this species.

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