Detection of the linear SiC and SiC radicals in IRC\,+10216
arXiv:2508.04509 · doi:10.1051/0004-6361/202556370
Abstract
We detected the linear radicals SiC and SiC toward IRC+10216 using an ultrasensitive line survey gathered with the Yebes 40\,m radio telescope. The derived column densities of -SiC and -SiC are (3.60.4)10 cm and (1.80.2)10 cm, respectively. The linear SiC radical is 2 times less abundant that its singlet rhomboidal prolate isomer, for which we provide a new analysis based on recent sensitive observations in the Q band (7\,mm), and at 3 and 2\,mm with the IRAM 30m telescope. The emission detected from these species arises from the cool external layers of the circumstellar envelope. We speculate whether ion-neutral routes involving SiCH cations or neutral-neutral reactions involving Si and SiC could efficiently synthesize these species.
Letter accepted for publication in Astronomy & Astrophysics
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