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Table · dataset · 2020

Propargylimine in laboratory and in space

Listed in IVOA Registry (Virtual Observatory)

Small imines containing up to three carbon atoms are present in the interstellar medium.

Description

As alkynyl compounds are abundant in this medium, propargylimine (2-propyn-1-imine, HC=C-CH=NH) thus represents a promising candidate for a new interstellar detection. The goal of the present work is to perform a comprehensive laboratory investigation of the rotational spectrum of propargylimine in its ground vibrational state in order to obtain a highly precise set of rest-frequencies and to search it in space.

The rotational spectra of E and Z geometrical isomers of propargylimine have been recorded in laboratory in the 83-500GHz frequency interval. The measurements have been performed using a source-modulation millimetre-wave spectrometer equipped with a pyrolysis system for the production of unstable species. High-level ab initio calculations were performed to assist the analysis and to obtain reliable estimates for an extended set of spectroscopic quantities.

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We have searched for propargylimine at 3 and 2mm in the spectral survey of the quiescent giant molecular cloud G+0.693-0.027 located in the "Central Molecular Zone", close to the Galactic Centre. About 1000 rotational transitions have been recorded for the E- and Z-propargylimine, in the laboratory. These new data have enabled the determination of a very accurate set of spectroscopic parameters including rotational, quartic and sextic centrifugal distortion constants.

The improved spectral data allow us to perform a successful search for this new imine in the G+0.693-0.027 molecular cloud. Eighteen lines of Z-propargylimine have been detected at level >2.5*sigma, resulting in a column density estimate of N=(0.24+/-0.02)x10^-14^cm^-2^. An upper limit was retrieved for the higher-energy E isomer, which was not detected in the data.

The fractional abundance (w.r.t. H_2_) derived for Z-propargylimine is 1.8x10^-10^. We discuss the possible formation routes by comparing the derived abundance with those measured in the source for possible chemical precursors.

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Catalogue records · 2

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Provenance · 1 source records, 7 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/640/a9815 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0