Detection of the linear SiC<sub>3</sub> and SiC<sub>5</sub> radicals in IRC+10216

We detected the linear 3 Σ − radicals SiC 3 and SiC 5 toward IRC+10216 using an ultrasensitive line survey gathered with the Yebes 40 m radio telescope. The derived column densities of l -SiC 3 and l -SiC 5 are (3.6 ± 0.4) × 10 12 cm −2 and (1.8 ± 0.2) × 10 12 cm −2 , respectively. The linear SiC 3 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 30 m telescope. The emission detected from these species arises from the cool external layers of the circumstellar envelope. We speculate whether ion-neutral routes involving SiC n H m + cations or neutral-neutral reactions involving Si and SiC 2 could efficiently synthesize these species.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-08-01
DOI
https://doi.org/10.1051/0004-6361/202556370
Citations
2
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
2.31

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article

Detection of the linear SiC3 and SiC5 radicals in IRC+10216

L. Velilla-Prieto, P. de Vicente, M. Guélin, J. R. Pardo et al.
2 citations
Astronomy and Astrophysics
Astrophysics and Star Formation Studies
2.31
article

Detection of the linear SiC3 and SiC5 radicals in IRC+10216

L. Velilla-Prieto, P. de Vicente, M. Guélin, J. R. Pardo, M. Agúndez, J. P. Fonfría, J. Cernicharo, C. Cabezas, B. Tercero
article en
2 citations

Abstract

We detected the linear 3 Σ − radicals SiC 3 and SiC 5 toward IRC+10216 using an ultrasensitive line survey gathered with the Yebes 40 m radio telescope. The derived column densities of l -SiC 3 and l -SiC 5 are (3.6 ± 0.4) × 10 12 cm −2 and (1.8 ± 0.2) × 10 12 cm −2 , respectively. The linear SiC 3 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 30 m telescope. The emission detected from these species arises from the cool external layers of the circumstellar envelope. We speculate whether ion-neutral routes involving SiC n H m + cations or neutral-neutral reactions involving Si and SiC 2 could efficiently synthesize these species.

Astronomy and AstrophysicsVol. 700
Instituto de Física Fundamental (ES), Institut de Radioastronomie Millimétrique (FR), Yebes Observatory (ES), Spanish National Observatory (ES)
European Research Council, Agencia Estatal de Investigación, European Social Fund
Openalex Percentile: Top 11%
Astrophysics and Star Formation Studies
2.31
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