Detection of the CN Zeeman effect in molecular clouds

被引:119
作者
Crutcher, RM [1 ]
Troland, TH
Lazareff, B
Paubert, G
Kazès, I
机构
[1] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
[2] Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA
[3] Domaine Univ, Inst Radioastron Millimetr, F-38406 St Martin Dheres, France
[4] Inst Radio Astron Millimetr, E-18012 Granada, Spain
[5] Observ Paris, Meudon Sect, F-92195 Meudon, France
基金
美国国家科学基金会;
关键词
ISM : clouds; ISM : magnetic fields; stars : formation;
D O I
10.1086/311952
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observations of the Zeeman effect in the 3 mm lines of CN have been carried out with the 30 m IRAM telescope toward seven dense molecular clouds. Detections were achieved toward the Orion Molecular Cloud 1 (OMC1), toward two cores in the DR21OH molecular cloud, and probably toward the M17SW molecular cloud. The line-of-sight magnetic field strengths inferred are B-los(OMC1)= -0.36 +/- 0.08, B-los(DR21OH(1)) = -0.36 +/- 0.10, B-los(DR210H(2)) = -0.71 +/- 0.12, and B-los(M17SW) = -0.33 +/- 0.14 mG. The theoretical implications of these results are discussed.
引用
收藏
页码:L121 / L124
页数:4
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