The submillimeter-wave spectrum of ...
Document type :
Compte-rendu et recension critique d'ouvrage
Title :
The submillimeter-wave spectrum of diisocyanomethane
Author(s) :
Motiienko, Roman [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Margulès, Laurent [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Guillemin, Jean-Claude [Auteur]
Institut des Sciences Chimiques de Rennes [ISCR]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Margulès, Laurent [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Guillemin, Jean-Claude [Auteur]
Institut des Sciences Chimiques de Rennes [ISCR]
Journal title :
Astronomy and Astrophysics - A&A
Pages :
82
Publisher :
EDP Sciences
Publication date :
2012-08
ISSN :
0004-6361
English keyword(s) :
ISM: molecules
methods: laboratory
submillimeter: ISM
molecular data
line: identification
methods: laboratory
submillimeter: ISM
molecular data
line: identification
HAL domain(s) :
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Chimie/Chimie organique
Chimie/Chimie organique
English abstract : [en]
Context. Several organic isocyanides (HNC, CH3NC, HCCNC) have been observed to date in the interstellar medium (ISM). However there is still a lack of high-resolution spectroscopic data for simple isocyanides that could ...
Show more >Context. Several organic isocyanides (HNC, CH3NC, HCCNC) have been observed to date in the interstellar medium (ISM). However there is still a lack of high-resolution spectroscopic data for simple isocyanides that could provide a basis for their detection. Aims: Diisocyanomethane (CNCH2NC) is a small molecule with only seven atoms that is an interesting candidate for astrophysical detection. The rotational spectrum of diisocyanomethane has never been studied before, hence we present our analysis of its spectrum. Methods: We measured the rotational spectrum of diisocyanomethane in the frequency range 120-620 GHz using the Lille fast-scan and solid-state source spectrometers. The spectroscopic study was supported by high-level theoretical calculations of the molecular structure and both the harmonic and anharmonic force field. Results: The ground and the first excited vibrational state (ν15) are assigned and analysed. The dataset is composed of more than 2000 measured and fitted lines, which allows us to make accurate predictions of transition frequencies of diisocyanomethane in the frequency range up to 900 GHz. The statistical analysis of the results of the fit shows that the use of the S-reduction of the Watson rovibrational Hamiltonian for spectral modelling is more appropriate. Full Tables 2 and 3 are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/544/A82Show less >
Show more >Context. Several organic isocyanides (HNC, CH3NC, HCCNC) have been observed to date in the interstellar medium (ISM). However there is still a lack of high-resolution spectroscopic data for simple isocyanides that could provide a basis for their detection. Aims: Diisocyanomethane (CNCH2NC) is a small molecule with only seven atoms that is an interesting candidate for astrophysical detection. The rotational spectrum of diisocyanomethane has never been studied before, hence we present our analysis of its spectrum. Methods: We measured the rotational spectrum of diisocyanomethane in the frequency range 120-620 GHz using the Lille fast-scan and solid-state source spectrometers. The spectroscopic study was supported by high-level theoretical calculations of the molecular structure and both the harmonic and anharmonic force field. Results: The ground and the first excited vibrational state (ν15) are assigned and analysed. The dataset is composed of more than 2000 measured and fitted lines, which allows us to make accurate predictions of transition frequencies of diisocyanomethane in the frequency range up to 900 GHz. The statistical analysis of the results of the fit shows that the use of the S-reduction of the Watson rovibrational Hamiltonian for spectral modelling is more appropriate. Full Tables 2 and 3 are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/544/A82Show less >
Language :
Anglais
Popular science :
Non
Source :
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