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Decoding millimetre-wave spectra of 2-iminopropanenitrile, a candidate for astronomical observations

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F60461373%3A22340%2F22%3A43923986" target="_blank" >RIV/60461373:22340/22:43923986 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.aanda.org/articles/aa/full_html/2022/09/aa43696-22/aa43696-22.html" target="_blank" >https://www.aanda.org/articles/aa/full_html/2022/09/aa43696-22/aa43696-22.html</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202243696" target="_blank" >10.1051/0004-6361/202243696</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Decoding millimetre-wave spectra of 2-iminopropanenitrile, a candidate for astronomical observations

  • Original language description

    Aims. The recent detection of cyanomethanimine in the interstellar medium makes its methyl derivative, 2-iminopropanenitrile (CH3C(CN)NH), a promising candidate for an interstellar detection. The aim of this work is to extend the current knowledge of the laboratory rotational spectrum to higher frequencies, which is an essential prerequisite for an identification of the molecular species in the interstellar medium by millimetre-wave astronomy.Methods. The room-temperature rotational spectrum of 2-iminopropanenitrile has been measured in several frequency regions between 128 and 329 GHz. The A–E splittings of the rotational transitions arising from the methyl top internal rotation were analysed employing the ERHAM and XIAM programs.Results. A dataset of approximately 900 newly assigned rotational transitions in the ground state of the Z isomer and a set of refined molecular constants, including the internal rotation parameters, are reported. Moreover, this work provides the first spectral characterisation of the less stable E isomer ground state, as well as the three lowest-lying vibrationally excited states of the Z isomer, v21 = 1, v14 = 1, and v20 = 1. This comprehensive spectroscopic study will allow a search for 2-iminopropanenitrile in the millimetre-wave surveys of interstellar sources, such as those recorded by the Atacama Large Millimeter/submillimeter Array.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10403 - Physical chemistry

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    ASTRONOMY &amp; ASTROPHYSICS

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    665

  • Issue of the periodical within the volume

    September 2022

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    10

  • Pages from-to

    "A9"

  • UT code for WoS article

    000849046800006

  • EID of the result in the Scopus database

    2-s2.0-85138301521