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The interstellar chemistry of H2C3O isomers

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 22 Jan 2016Embargo end date: 01 Jan 2015 France, Spain English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 456, pages 4,101-4,110 (issn: 0035-8711, eissn: 1365-2966, Copyright policy )Funded by:EC | NANOCOSMOS, EC | 3DICE
Authors: Loison, Jean-Christophe,; Agúndez, Marcelino,; Marcelino, Núria,; Wakelam, Valentine; Hickson, Kevin M.,; Cernicharo, José,; Gerin, Maryvonne,; +2 Authors

doi: 10.1093/mnras/stv2866 , 10.48550/arxiv.1512.01582

pmid: 27013768

pmc: PMC4803190

arXiv: 1512.01582

handle: 10261/186550

The interstellar chemistry of H2C3O isomers

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.

19 pages, 4 Figures, 4 Tables

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France, Spain
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Keywords

[SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 500, FOS: Physical sciences, 540, ISM: clouds, Astrophysics - Astrophysics of Galaxies, ISM: molecules, ISM: clouds - ISM: molecules, Astrophysics of Galaxies (astro-ph.GA), clouds [ISM], molecules [ISM]

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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