4.7 Article

The interstellar chemistry of H2C3O isomers

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 456, Issue 4, Pages 4101-4110

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv2866

Keywords

ISM: clouds; ISM: molecules

Funding

  1. French CNRS/INSU program PCMI
  2. ERC Starting Grant (3DICE) [336474]
  3. European Research Council (ERC) [610256: NANOCOSMOS]
  4. Spanish MINECO [CSD2009-00038, AYA2009-07304, AYA2012-32032]

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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.

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