An Observational Investigation of the Identity of B11244 (l-C3H+/C3H-)
Abstract
Pety et al. have reported the detection of eight transitions of a closed-shell, linear molecule (B11244) in observations toward the Horsehead photodissociation region (PDR), which they attribute to the l-C3H+ cation. Recent high-level ab initio calculations have called this assignment into question; the anionic C3H- molecule has been suggested as a more likely candidate. Here, we examine observations of the Horsehead PDR, Sgr B2(N), TMC-1, and IRC+10216 in the context of both l-C3H+ and C3H-. We find no observational evidence of Ka = 1 lines, which should be present were the carrier indeed C3H-. Additionally, we find a strong anticorrelation between the presence of known molecular anions and B11244 in these regions. Finally, we discuss the formation and destruction chemistry of C3H- in the context of the physical conditions in the regions. Based on these results, we conclude there is little evidence to support the claim that the carrier is C3H-.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- March 2014
- DOI:
- arXiv:
- arXiv:1312.0153
- Bibcode:
- 2014ApJ...783...36M
- Keywords:
-
- astrochemistry;
- ISM: clouds;
- ISM: individual objects: Sagittarius B2(N) TMC-1 Horsehead PDR IRC+10216;
- ISM: molecules;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 17 pages, 3 figures, accepted in the Astrophysical Journal