Search for anions in molecular sources:: C4H- detection in L1527

被引:104
作者
Agundez, M. [1 ]
Cernicharo, J. [1 ]
Guelin, M. [2 ]
Gerin, M. [3 ,4 ]
McCarthy, M. C. [5 ]
Thaddeus, P. [5 ]
机构
[1] CSIC, Ist Estructura Mat, Dept Astrofis Mol & Infrarroja, Madrid 28006, Spain
[2] Inst Radio Astron Millimetr, F-38406 St Martin Dheres, France
[3] Observ Paris, UMR CNRS 8112, LERMA, F-75231 Paris, France
[4] Ecole Normale Super, F-75231 Paris, France
[5] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
astrochemistry; ISM : molecules; radio lines : ISM;
D O I
10.1051/0004-6361:20078985
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We present the results of a search for the negative ion C4H- in various dark clouds, low mass star-forming regions and photon-dominated regions (PDRs). We have also searched for C6H-, C2H- and CN- in some of the sources. Methods. The millimeter-wave observations were carried out with the IRAM-30 m telescope. Results. We detect C4H-, through the J = 9-8 and J = 10-9 rotational transitions, in the low mass star-forming region L1527. We thus confirm the tentative detection of the J = 9-8 line recently reported toward this source. The [C4H-]/[C4H] ratio found is 0.011%, which is slightly lower than the value observed in IRC + 10216, 0.024%, but above the 3 sigma upper limit we derive in TMC-1, < 0.0052%. We have also derived an upper limit for the [C6H-]/[C6H] ratio in the Horsehead Nebula, and for various anion-to-neutral ratios in the observed sources. These results are compared with recent chemical models.
引用
收藏
页码:L19 / L22
页数:4
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