Laboratory detection of the carbon chains HC15N and HC17N

被引:56
作者
McCarthy, MC
Grabow, JU
Travers, MJ
Chen, W
Gottlieb, CA
Thaddeus, P
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] Harvard Univ, Div Engn & Appl Sci, Cambridge, MA 02138 USA
关键词
ISM; molecules; line; identification; molecular data; molecular processes; radio lines ISM;
D O I
10.1086/311188
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The linear cyanopolyynes HC(15)N and HC(17)N were detected in the laboratory by Fourier transform microwave spectroscopy. Enough rotational lines of each species were measured in the 5-11 GHz frequency range so that precise values for the rotational and centrifugal distortion constants can be determined and the entire rotational spectra of both molecules predicted to better than 1 km s(-1) in equivalent radial velocity over the range of interest to radio astronomy. Although there is a nearly constant decrement in line intensity from HC(3)N to HC(9)N of about seven, the decrement decreases by at least a factor of 2 on reaching HC(17)N, and as a result the lines of HC(17)N are nearly an order of magnitude stronger than predicted by extrapolation from the shorter cyanopolyynes. With a molecular weight of 219 amu and a rotational constant of slightly more than 50 MHz, HC(17)N is the longest carbon chain identified to date by high-resolution spectroscopy.
引用
收藏
页码:L231 / L234
页数:4
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