A Search for l-C3H+ and l-C3H in Sgr B2(N), Sgr B2(OH), and the Dark Cloud TMC-1
Abstract
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+.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- September 2013
- DOI:
- arXiv:
- arXiv:1307.2173
- Bibcode:
- 2013ApJ...774...56M
- Keywords:
-
- astrochemistry;
- ISM: clouds;
- ISM: individual objects: Sagittarius B2(N) Sagittarius B2(OH) TMC-1;
- ISM: molecules;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 17 Pages, 6 Figures, Accepted in The Astrophysical Journal