A 8.8-50 GHz complete spectral line survey toward TMC-1 I. Survey data

被引:162
|
作者
Kaifu, N [1 ]
Ohishi, M
Kawaguchi, K
Saito, S
Yamamoto, S
Miyaji, T
Miyazawa, K
Ishikawa, S
Noumaru, C
Harasawa, S
Okuda, M
Suzuki, H
机构
[1] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[2] Natl Astron Observ Japan, Astron Data Anal Ctr, Mitaka, Tokyo 1818588, Japan
[3] Okayama Univ, Fac Sci, Dept Chem, Okayama 7008530, Japan
[4] Univ Fukui, Res Ctr Dev Far Infrared Region, Bunkyo Ku, Fukui, Fukui 9108507, Japan
[5] Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, Tokyo 1130033, Japan
[6] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
[7] Natl Astron Observ Japan, Nobeyama Radio Observ, Nagano 3841305, Japan
[8] Natl Astron Observ Japan, Subaru Telescope Facil, Hilo, HI 96740 USA
关键词
ISM : abundances; ISM : individual (TMC-1); ISM : molecules;
D O I
10.1093/pasj/56.1.69
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We completed the first spectral line survey toward a cold, dark cloud TMC-1 (cyanopolyyne peak) in a frequency range between 8.8 and 50.0 GHz by the 45-m radio telescope of Nobeyama Radio Observatory. We detected 414 lines of 38 molecular species including 11 new molecules, such as C6H, CCO, C3O, CCS, C3S, HNCCC, HCCNC, HC3NH+, HCCCHO, CH2CN, and cyclic C3H (c-C3H), which were previously reported; only one significant line. U49536, remains unidentified. 177 out of 414 lines are reported for the first time. Some half of the detected molecules are linear carbon-chain species and their derivatives. We also discovered three new rarer isotopomers: (CCS)-S-34 (C3S)-S-34, and HDCS. Spectral charts are presented together with the observed line parameters of all detected lines. Improved molecular constants of several carbon-chain molecules obtained during the course of identification are also presented.
引用
收藏
页码:69 / 173
页数:105
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