Searching for trans ethyl methyl ether in Orion KL

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Abstract

We report on the tentative detection of trans ethyl methyl ether (tEME), t-CH3CH2OCH3, through the identification of a large number of rotational lines from each one of the spin states of the molecule towards Orion KL. We also search for gauche-trans-n-propanol, Gt-n-CH3CH2CH2OH, an isomer of tEME in the same source. We have identified lines of both species in the IRAM 30 m line survey and in the ALMA Science Verification data. We have obtained ALMA maps to establish the spatial distribution of these species. Whereas tEME mainly arises from the compact ridge component of Orion, Gt-n-propanol appears at the emission peak of ethanol (south hot core). The derived column densities of these species at the location of their emission peaks are < (4.0 +0.8) 1015cm2and

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Tercero, B., Cernicharo, J., López, A., Brouillet, N., Kolesniková, L., Motiyenko, R. A., … Guillemin, J. C. (2015). Searching for trans ethyl methyl ether in Orion KL. Astronomy and Astrophysics, 582. https://doi.org/10.1051/0004-6361/201526255

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