{ "id": "1906.06508", "version": "v1", "published": "2019-06-15T09:23:21.000Z", "updated": "2019-06-15T09:23:21.000Z", "title": "Synthesis of solid-state Complex Organic Molecules through accretion of simple species at low temperatures", "authors": [ "D. Qasim", "G. Fedoseev", "K. -J. Chuang", "V. Taquet", "T. Lamberts", "J. He", "S. Ioppolo", "E. F. van Dishoeck", "H. Linnartz" ], "comment": "Proceedings IAU Symposium No. 350, 2019, Laboratory Astrophysics: from Observations to Interpretation", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "Complex organic molecules (COMs) have been detected in the gas-phase in cold and lightless molecular cores. Recent solid-state laboratory experiments have provided strong evidence that COMs can be formed on icy grains through 'non-energetic' processes. In this contribution, we show that propanal and 1-propanol can be formed in this way at the low temperature of 10 K. Propanal has already been detected in space. 1-propanol is an astrobiologically relevant molecule, as it is a primary alcohol, and has not been astronomically detected. Propanal is the major product formed in the C2H2 + CO + H experiment, and 1-propanol is detected in the subsequent propanal + H experiment. The results are published in Qasim et al. (2019c). ALMA observations towards IRAS 16293-2422B are discussed and provide a 1-propanol:propanal upper limit of < 0.35 - 0.55, which are complemented by computationally-derived activation barriers in addition to the performed laboratory experiments.", "revisions": [ { "version": "v1", "updated": "2019-06-15T09:23:21.000Z" } ], "analyses": { "keywords": [ "solid-state complex organic molecules", "low temperature", "simple species", "solid-state laboratory experiments", "propanal upper limit" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }