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Published in

Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 4(456), p. 4101-4110

DOI: 10.1093/mnras/stv2866

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The interstellar chemistry of H2C3O isomers

This paper is available in a repository.
This paper is available in a repository.

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Postprint: archiving allowed
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Data provided by SHERPA/RoMEO

Abstract

We present the detection of two H2C3O isomers, propynal and cyclopropenone, toward various starless cores and molecular clouds, together with upper limits for the third isomer propadienone. We review the processes controlling the abundances of H2C3O isomers in interstellar media showing that the reactions involved are gas-phase ones. We show that the abundances of these species are controlled by kinetic rather than thermodynamic effects.