Microwave and submillimeter spectroscopy ...
Type de document :
Compte-rendu et recension critique d'ouvrage
Titre :
Microwave and submillimeter spectroscopy and first ISM detection of 18O-methyl formate
Auteur(s) :
Tercero, B., [Auteur]
Centro de Astrobiologia [Madrid] [CAB]
Margulès, Laurent [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Carvajal, M., [Auteur]
Universidad de Huelva
Motiienko, Roman [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Huet, Therese [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Alekseev, E. A. [Auteur]
Institute of Radio Astronomy of NAS of Ukraine [IRA]
Kleiner, I. [Auteur]
Laboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
Guillemin, Jean-Claude [Auteur]
Institut des Sciences Chimiques de Rennes [ISCR]
Møllendal, Harald [Auteur]
Centre for Theoretical and Computational Chemistry [Oslo] [CTCC]
Cernicharo, J., [Auteur]
Centro de Astrobiologia [Madrid] [CAB]
Centro de Astrobiologia [Madrid] [CAB]
Margulès, Laurent [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Carvajal, M., [Auteur]
Universidad de Huelva
Motiienko, Roman [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Huet, Therese [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Alekseev, E. A. [Auteur]
Institute of Radio Astronomy of NAS of Ukraine [IRA]
Kleiner, I. [Auteur]
Laboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
Guillemin, Jean-Claude [Auteur]
Institut des Sciences Chimiques de Rennes [ISCR]
Møllendal, Harald [Auteur]
Centre for Theoretical and Computational Chemistry [Oslo] [CTCC]
Cernicharo, J., [Auteur]
Centro de Astrobiologia [Madrid] [CAB]
Titre de la revue :
Astronomy and Astrophysics - A&A
Pagination :
119
Éditeur :
EDP Sciences
Date de publication :
2012-02
ISSN :
0004-6361
Mot(s)-clé(s) en anglais :
submillimeter: ISM
line: identification
astronomical databases: miscellaneous
ISM: individual objects: Orion KL
ISM: molecules
astrochemistry
line: identification
astronomical databases: miscellaneous
ISM: individual objects: Orion KL
ISM: molecules
astrochemistry
Discipline(s) HAL :
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Chimie/Chimie organique
Chimie/Chimie théorique et/ou physique
Physique [physics]/Physique Quantique [quant-ph]
Physique [physics]/Physique [physics]/Physique Atmosphérique et Océanique [physics.ao-ph]
Planète et Univers [physics]
Chimie/Chimie organique
Chimie/Chimie théorique et/ou physique
Physique [physics]/Physique Quantique [quant-ph]
Physique [physics]/Physique [physics]/Physique Atmosphérique et Océanique [physics.ao-ph]
Planète et Univers [physics]
Résumé en anglais : [en]
Context. Astronomical survey of interstellar molecular clouds needs a previous analysis of the spectra in the microwave and sub-mm energy range to be able to identify them. We obtained very accurate spectroscopic constants ...
Lire la suite >Context. Astronomical survey of interstellar molecular clouds needs a previous analysis of the spectra in the microwave and sub-mm energy range to be able to identify them. We obtained very accurate spectroscopic constants in a comprehensive laboratory analysis of rotational spectra. These constants can be used to predict transition frequencies that were not measured in the laboratory very precisely. Aims: We present an experimental study and a theoretical analysis of two 18O-methyl formate isotopologues, which were subsequently detected for the first time in Orion KL. Methods: The experimental spectra of both methyl formate isotopologues recorded in the microwave and sub-mm range from 1 to 660 GHz. Both spectra were analysed by using the rho-axis method (RAM) which takes into account the CH3 internal rotation. Results: We obtained spectroscopic constants of both 18O- methyl formate with high accuracy. Thousands of transitions were assigned and others predicted, which allowed us to detect both species in the IRAM 30 m line survey of Orion KL. Full Tables A.1 et A.2 are 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/538/A119Lire moins >
Lire la suite >Context. Astronomical survey of interstellar molecular clouds needs a previous analysis of the spectra in the microwave and sub-mm energy range to be able to identify them. We obtained very accurate spectroscopic constants in a comprehensive laboratory analysis of rotational spectra. These constants can be used to predict transition frequencies that were not measured in the laboratory very precisely. Aims: We present an experimental study and a theoretical analysis of two 18O-methyl formate isotopologues, which were subsequently detected for the first time in Orion KL. Methods: The experimental spectra of both methyl formate isotopologues recorded in the microwave and sub-mm range from 1 to 660 GHz. Both spectra were analysed by using the rho-axis method (RAM) which takes into account the CH3 internal rotation. Results: We obtained spectroscopic constants of both 18O- methyl formate with high accuracy. Thousands of transitions were assigned and others predicted, which allowed us to detect both species in the IRAM 30 m line survey of Orion KL. Full Tables A.1 et A.2 are 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/538/A119Lire moins >
Langue :
Anglais
Vulgarisation :
Non
Source :
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