Laboratory and radio-astronomical spectroscopy of the hyperfine structure of N2D+

被引:38
作者
Dore, L
Caselli, P
Beninati, S
Bourke, T
Myers, PC
Cazzoli, G
机构
[1] Univ Bologna, Dipartimento Chim G Ciamician, I-40126 Bologna, Italy
[2] Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
molecular data; methods : laboratory; ISM : individual : L183; molecules; radio lines : ISM;
D O I
10.1051/0004-6361:20034025
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first laboratory measurements of the hyperfine structure of the J = 1 <-- 0 rotational transition of N2D+, a good tracer of the dense regions of molecular cloud cores, and the spectra of unresolved high J transitions recorded in the 308-463 GHz region. Together with a high sensitivity radio-astronomical spectrum of the N2D+ J = 1 --> 0 rotational transition in a quiescent cloud core, we determined with high precision the frequencies of the seven hyperfine components and the molecular spectroscopic constants, allowing us to make predictions on the N2D+ frequencies of higher J transitions occurring in the submillimeter-wave region.
引用
收藏
页码:1177 / 1181
页数:5
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