Hunting for hot corinos and WCCC sources in the OMC-2/3 filament

13 Mar 2020 Bouvier M. López-Sepulcre A. Ceccarelli C. Kahane C. Imai M. Sakai N. Yamamoto S. Dagdigian P. J.

Context: Solar-like protostars are known to be chemically rich, but it is not yet clear how much their chemical composition can vary and why. So far, two chemically distinct types of Solar-like protostars have been identified: hot corinos, which are enriched in interstellar Complex Organic Molecules (iCOMs), such as methanol (CH$_3$OH) or dimethyl ether (CH$_3$OCH$_3$), and Warm Carbon Chain Chemistry (WCCC) objects, which are enriched in carbon chain molecules, such as butadiynyl (C$_4$H) or ethynyl radical (CCH)... (read more)

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