Abstract
Seven rotational transitions of SiC 3 , a planar, highly polar ring molecule, have been detected in the millimeter-wave band in the expanding envelope of the evolved carbon star IRC ϩ10216. On the assumption that SiC 3 has the same 40Љ diameter shell as SiCC, the mean column density of SiC 3 is cm . The rotational 12 Ϫ2 4.3 # 10 excitation of SiC 3 is similar to that of SiCC, with a low rotational temperature within the K-stacks of 10–20 K and a high rotational temperature across the K-stacks of roughly 50 K, which is probably close to the kinetic temperature of the shell.
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CITATION STYLE
Apponi, A. J., McCarthy, M. C., Gottlieb, C. A., & Thaddeus, P. (1999). Astronomical Detection of Rhomboidal S[CLC]i[/CLC]C[TINF]3[/TINF]. The Astrophysical Journal, 516(2), L103–L106. https://doi.org/10.1086/311998
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