{ "id": "2308.09459", "version": "v1", "published": "2023-08-18T10:46:25.000Z", "updated": "2023-08-18T10:46:25.000Z", "title": "The first detection of SiC$_2$ in the interstellar medium", "authors": [ "S. Massalkhi", "I. Jiménez-Serra", "J. Martín-Pintado", "V. M. Rivilla", "L. Colzi", "S. Zeng", "S. Martín", "B. Tercero", "P. de Vicente", "M. A. Requena-Torres" ], "comment": "8 pages, 5 figures", "categories": [ "astro-ph.GA" ], "abstract": "We report the first detection of SiC$_2$ in the interstellar medium. The molecule was identified through six rotational transitions toward G\\,+0.693$-$0.027, a molecular cloud located in the Galactic center. The detection is based on a line survey carried out with the GBT, the Yebes 40m, and the IRAM 30m telescopes covering a range of frequencies from 12 to 276 GHz. We fit the observed spectra assuming local thermodynamic equilibrium and derive a column density of ($1.02\\pm0.04)\\times10^{13}$ cm$^{-2}$, which gives a fractional abundance of $7.5\\times10^{-11}$ with respect to H$_2$, and an excitation temperature of $5.9\\pm0.2$ K. We conclude that SiC$_2$ can be formed in the shocked gas by a reaction between the sputtered atomic silicon and C$_2$H$_2$, or it can be released directly from the dust grains due to disruption. We also search for other Si-bearing molecules and detect eight rotational transitions of SiS and four transitions of Si$^{18}$O. The derived fractional abundances are $3.9\\times10^{-10}$ and $2.1\\times10^{-11}$, respectively. All Si-bearing species toward G\\,+0.693$-$0.027 show fractional abundances well below what is typically found in late-type evolved stars.", "revisions": [ { "version": "v1", "updated": "2023-08-18T10:46:25.000Z" } ], "analyses": { "keywords": [ "interstellar medium", "first detection", "fractional abundance", "rotational transitions", "spectra assuming local thermodynamic equilibrium" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable" } } }