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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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