AN OBSERVATIONAL INVESTIGATION OF THE IDENTITY OF B11244 (l-C3H+/C3H-)

被引:19
|
作者
McGuire, Brett A. [1 ]
Carroll, P. Brandon [1 ]
Gratier, Pierre [2 ,3 ,4 ]
Guzman, Viviana [2 ]
Pety, Jerome [2 ,3 ,4 ]
Roueff, Evelyne [5 ,6 ,7 ,8 ]
Gerin, Maryvonne [3 ,4 ]
Blake, Geoffrey A. [1 ,9 ]
Remijan, Anthony J. [10 ]
机构
[1] CALTECH, Div Chem & Chem Engn, Pasadena, CA 91125 USA
[2] Inst Radio Astron Millimetr, F-38406 St Martin Dheres, France
[3] CNRS, LERMA, UMR 8112, F-75014 Paris, France
[4] Observ Paris, F-75014 Paris, France
[5] CNRS, LUTH, UMR 8102, F-92195 Meudon, France
[6] Observ Paris, F-92195 Meudon, France
[7] CNRS, LERMA, UMR 8112, F-92190 Meudon, France
[8] Observ Paris, F-92190 Meudon, France
[9] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[10] Natl Radio Astron Observ, Charlottesville, VA 22903 USA
关键词
astrochemistry; ISM: clouds; ISM: individual objects (Sagittarius B2(N); TMC-1; Horsehead PDR; IRC+10216); ISM: molecules; GREEN-BANK TELESCOPE; NEBULA PHOTODISSOCIATION REGION; STAR-FORMING REGIONS; HORSEHEAD NEBULA; ASTRONOMICAL IDENTIFICATION; VIBRATIONAL FREQUENCIES; SPECTROSCOPIC CONSTANTS; ELECTRON-ATTACHMENT; MOLECULAR CLOUDS; LINE SURVEY;
D O I
10.1088/0004-637X/783/1/36
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 K-a = 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-.
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页数:7
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