Pety et al. recently reported the detection of several transitions of an unknown carrier in the Horsehead PDR and attribute them to l-C3H +. Here, we have tested the predictive power of their fit by searching for, and identifying, the previously unobserved J = 1-0 and J = 2-1 transitions of the unknown carrier (B11244) toward Sgr B2(N) in data from the publicly available PRIMOS project. Also presented here are observations of the J = 6-5 and J = 7-6 transitions toward Sgr B2(N) and Sgr B2(OH) using the Barry E. Turner Legacy Survey and results from the Kaifu et al. survey of TMC-1. We calculate an excitation temperature and column density of B11244 of 10 K and ∼1013 cm-2 in Sgr B2(N) and ∼79 K with an upper limit of ≤1.5 × 1013 cm-2 in Sgr B2(OH) and find trace evidence for the cation's presence in TMC-1. Finally, we present spectra of the neutral species in both Sgr B2(N) and TMC-1, and comment on the robustness of the assignment of the detected signals to l-C3H +. © 2013. The American Astronomical Society. All rights reserved.
CITATION STYLE
McGuire, B. A., Carroll, P. B., Loomis, R. A., Blake, G. A., Hollis, J. M., Lovas, F. J., … Remijan, A. J. (2013). A search for l-C3H+ and l-C3H in Sgr B2(N), Sgr B2(OH), and the dark cloud TMC-1. Astrophysical Journal, 774(1). https://doi.org/10.1088/0004-637X/774/1/56
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