Literature DB >> 11034851

The Millimeter- and Submillimeter-Wave Spectrum of HC(3)N in the Ground and Vibrationally Excited States.

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Abstract

The pure rotational spectrum of the astrophysically very important linear molecule cyanoacetylene, HC(3)N, in the ground and vibrationally excited states has been studied in selected regions from 118 to 814 GHz using the Cologne terahertz spectrometer. Vibrational satellites appendant to the following vibrational states have been recorded and analyzed (v(4), v(5), v(6), v(7)): (0, 0, 0, 1), (0, 0, 0, 2), (0, 0, 1, 0), (0, 0, 1, 1), (1, 0, 0, 0), (1, 0, 0, 1), and the Fermi resonance systems (0, 1, 0, 0)/(0, 0, 0, 3) and (1, 0, 0, 2)/(0, 2, 0, 0)(0e). With the exception of the latter resonance system, all states have been fitted within experimental accuracy. This work provides improved rest frequencies for the astronomical community and may also be beneficial in the improvement of global fits. Copyright 2000 Academic Press.

Entities:  

Year:  2000        PMID: 11034851     DOI: 10.1006/jmsp.2000.8209

Source DB:  PubMed          Journal:  J Mol Spectrosc        ISSN: 0022-2852            Impact factor:   1.507


  4 in total

1.  Discovery of HC4NC in TMC-1: A study of the isomers of HC3N, HC5N, and HC7N.

Authors:  J Cernicharo; N Marcelino; M Agúndez; C Bermúdez; C Cabezas; B Tercero; J R Pardo
Journal:  Astron Astrophys       Date:  2020-10-07       Impact factor: 5.802

2.  Discovery of HC3O+ in space: The chemistry of O-bearing species in TMC-1.

Authors:  J Cernicharo; N Marcelino; M Agúndez; Y Endo; C Cabezas; C Bermúdez; B Tercero; P de Vicente
Journal:  Astron Astrophys       Date:  2020-10-23       Impact factor: 5.802

3.  Complex organic molecules in strongly UV-irradiated gas.

Authors:  S Cuadrado; J R Goicoechea; J Cernicharo; A Fuente; J Pety; B Tercero
Journal:  Astron Astrophys       Date:  2017-07       Impact factor: 5.802

4.  The growth of carbon chains in IRC +10216 mapped with ALMA.

Authors:  M Agúndez; J Cernicharo; G Quintana-Lacaci; A Castro-Carrizo; L Velilla Prieto; N Marcelino; M Guélin; C Joblin; J A Martín-Gago; C A Gottlieb; N A Patel; M C McCarthy
Journal:  Astron Astrophys       Date:  2017-05       Impact factor: 5.802

  4 in total

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