Molecular Parameters for SiCN

NRAO National Radio Astronomy Observatory

SiCN is a linear radical with a X 2Π electronic ground state. Its rotational spectral lines appear as a series of lambda-doubled transitions with further splitting owing to lambda doubling and magnetic hyperfine structure. All three doublets lying within the upper portion of the atmospheric 3mm window were detected, though some were contaminated by other lines, in observations at the IRAM 30m telescope towards IRC+10216.


SiCN

D=2.9 D

Spectroscopic constants from Apponi, A. J., McCarthy, M. C., Gottlieb, C. A. & Thaddeus, P. 2000, ApJL, 536, L55:


Spectroscopic Constants of SiCCH, SiCN, and SiNC in the X 2Π State (in MHz)

ParameterSiCCHSiCNSiNC
A + γa...2169000(4000)2124000(6000)1763000(4000)
B...5436.6629(2)5543.4152(2)6396.6839(3)
D...0.0018244(5)0.0023102(2)0.0028890(4)
γa...1161(9)2070(10)2470(10)
p + 2q...32.071(2)25.734(2)9.800(3)
(p + 2q)D...-0.000420(7)-0.000386(7)0.01842(3)
q...0.807(4)0.869(2)1.385(7)
qD...-0.000016(2)...0.000011(7)
a - (b + c)/2...14.969(5)15.676(2)3.206(4)
b...-14.1(3)5.6(2)-5.2(3)
d...9.475(3)20.033(2)2.706(4)
eQq0......-5.031(3)-1.417(2)
eQq2......2.3(5)...
rms...0.0190.0320.034



Interstellar detection by Gu\'elin, Muller, Cernicharo, Apponi, McCarthy, Gottlieb and Thaddeus A&A 363, L9 2000.

Laboratory work by Apponi, A. J., McCarthy, M. C., Gottlieb, C. A. & Thaddeus, P. 2000, ApJL, 536, L55


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Known Interstellar Molecules Page