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On the Detection of Methoxymethanol, CH3OCH2OH, in Space
B. A. McGuire, C. N. Shingledecker, E. R. Willis, A. M. Burkhardt, S. El-Abd, R. A. Motiyenko, C. L. Brogan, T. R. Hunter, L. Margulès, J.-C. Guillemin, R. T. Garrod, E. Herbst, and A. J. Remijan,
reported on the
ALMA Detection of Interstellar Methoxymethanol (CH<sub>3</sub>OCH<sub>2</sub>OH),
Astrophys. J. 851 L46 (2017).
More than two dozen unblended or essentially unblended transitions were detected in several small recordings in Bands 6 and 7 through observations of the high-mass starforming region NGC 6334I-MM1. Assuming an excitation temperature of 200 K, its column density was found to be lower than that of methanol by a factor slightly larger than 30.
B. Tercero, S. Cuadrado, A. López, N. Brouillet, D. Despois, and J. Cernicharo
investigated
Chemical Segregation of Complex Organic O-bearing Species in Orion KL
Astron. Astrophys. 620, Art. No. L6 (2018).
They analyzed the Cycle 0 ALMA science verification data and found ethyl methyl ether besides several other molecules.
Contributor(s): H. S. P. Müller; 12, 2017; 07, 2019