{ "id": "2305.05073", "version": "v1", "published": "2023-05-08T22:21:22.000Z", "updated": "2023-05-08T22:21:22.000Z", "title": "An analysis of the isomers HCN and HNC in the evolution of high-mass star-forming regions", "authors": [ "N. C. Martinez", "S. Paron" ], "comment": "to appear in Bolet\\'in de la Asociaci\\'on Argentina de Astronom\\'ia", "categories": [ "astro-ph.GA" ], "abstract": "The study of molecules and their chemistry in star-forming regions is fundamental to understand the physical process occurring in such regions. The HCN and HNC J=1-0 emissions were used to derive their integrated line intensities (I), to probe a relation recently appeared in the literature between the kinetic temperatures (T$_{K}$) and the isomeric (I) ratio, and to obtain the isomers abundances (X) in 55 high-mass star-forming regions. These last ones are classified, according to the evolutive stage, as infrared dark clouds, high-mass protostellar objects, hot molecular cores, and ultracompact HII regions. It is inferred that the T$_{K}$ obtained from the isomeric integrated intensity ratio (I$^{HCN/HNC}$) are underestimated, and hence we suggest that this relation cannot be employed as an universal thermometer in the interstellar medium. The isomers abundances show a behavior that can be explained from the chemistry occurring as the temperature and the UV radiation increase according to the evolutive stage. We found that the abundance ratio (X$^{HCN/HNC}$) hardly could be used as a chemical clock, and we suggest that it can be approximated by I$^{HCN/HNC}$. This work is part of an on-going study of multiple molecules that stand in the sample of analyzed regions which intends to contribute in the chemical knowledge of high-mass star formation.", "revisions": [ { "version": "v1", "updated": "2023-05-08T22:21:22.000Z" } ], "analyses": { "keywords": [ "high-mass star-forming regions", "isomers hcn", "isomers abundances", "uv radiation increase", "ultracompact hii regions" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }