Hunting the relatives of benzonitrile: ...
Type de document :
Compte-rendu et recension critique d'ouvrage
Titre :
Hunting the relatives of benzonitrile: Rotational spectroscopy of dicyanobenzenes
Auteur(s) :
Chitarra, Olivia [Auteur]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Lee, Kin Long Kelvin [Auteur]
Massachusetts Institute of Technology [MIT]
Buchanan, Zachary [Auteur]
University of California [Davis] [UC Davis]
Melosso, Mattia [Auteur]
Alma Mater Studiorum Università di Bologna = University of Bologna [UNIBO]
Mcguire, Brett [Auteur]
Massachusetts Institute of Technology [MIT]
Goubet, Manuel [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Physique Moléculaire aux Interfaces [PMI]
Pirali, Olivier [Auteur]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Martin-Drumel, Marie-Aline [Auteur]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Lee, Kin Long Kelvin [Auteur]
Massachusetts Institute of Technology [MIT]
Buchanan, Zachary [Auteur]
University of California [Davis] [UC Davis]
Melosso, Mattia [Auteur]
Alma Mater Studiorum Università di Bologna = University of Bologna [UNIBO]
Mcguire, Brett [Auteur]
Massachusetts Institute of Technology [MIT]
Goubet, Manuel [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Physique Moléculaire aux Interfaces [PMI]
Pirali, Olivier [Auteur]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Martin-Drumel, Marie-Aline [Auteur]
Institut des Sciences Moléculaires d'Orsay [ISMO]
Titre de la revue :
Astronomy and Astrophysics - A&A
Pagination :
A163
Éditeur :
EDP Sciences
Date de publication :
2021-07-06
ISSN :
0004-6361
Mot(s)-clé(s) en anglais :
Methods
laboratory
molecular -techniques
spectroscopic -Astrochemistry -ISM
abundances -Submillimeter
general
laboratory
molecular -techniques
spectroscopic -Astrochemistry -ISM
abundances -Submillimeter
general
Discipline(s) HAL :
Physique [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Résumé en anglais : [en]
Context. The recent interstellar detections of-CN containing aromatic species, namely benzonitrile, 1-cyanonaphthalene, and 2cyanonaphthalene, bring renewed interest in related molecules that could participate in similar ...
Lire la suite >Context. The recent interstellar detections of-CN containing aromatic species, namely benzonitrile, 1-cyanonaphthalene, and 2cyanonaphthalene, bring renewed interest in related molecules that could participate in similar reaction networks. Aims. To enable new interstellar searches for benzonitrile derivatives, the pure rotational spectra of several related species need to be investigated in the laboratory. Methods. We have recorded the pure rotational spectra of ortho-and meta-dicyanobenzene in the centimetre and millimetre-wave domains. Assignments were supported by high-level quantum chemical calculations. Using Markov chain Monte Carlo simulations, we also searched for evidence of these molecules towards TMC-1 using the GOTHAM survey. Results. Accurate spectroscopic parameters are derived from the analysis of the experimental spectra, allowing for reliable predictions at temperatures of interest (i.e. 10-300 K) for astronomical searches. Our searches in TMC-1 for both ortho-and meta-isomers provide upper limits for the abundances of the species.Lire moins >
Lire la suite >Context. The recent interstellar detections of-CN containing aromatic species, namely benzonitrile, 1-cyanonaphthalene, and 2cyanonaphthalene, bring renewed interest in related molecules that could participate in similar reaction networks. Aims. To enable new interstellar searches for benzonitrile derivatives, the pure rotational spectra of several related species need to be investigated in the laboratory. Methods. We have recorded the pure rotational spectra of ortho-and meta-dicyanobenzene in the centimetre and millimetre-wave domains. Assignments were supported by high-level quantum chemical calculations. Using Markov chain Monte Carlo simulations, we also searched for evidence of these molecules towards TMC-1 using the GOTHAM survey. Results. Accurate spectroscopic parameters are derived from the analysis of the experimental spectra, allowing for reliable predictions at temperatures of interest (i.e. 10-300 K) for astronomical searches. Our searches in TMC-1 for both ortho-and meta-isomers provide upper limits for the abundances of the species.Lire moins >
Langue :
Anglais
Vulgarisation :
Non
Source :
Fichiers
- https://hal.archives-ouvertes.fr/hal-03292177/document
- Accès libre
- Accéder au document
- https://hal.archives-ouvertes.fr/hal-03292177/document
- Accès libre
- Accéder au document
- https://hal.archives-ouvertes.fr/hal-03292177/document
- Accès libre
- Accéder au document
- https://hal.archives-ouvertes.fr/hal-03292177/document
- Accès libre
- Accéder au document
- document
- Accès libre
- Accéder au document
- aa41386-21.pdf
- Accès libre
- Accéder au document
- document
- Accès libre
- Accéder au document
- aa41386-21.pdf
- Accès libre
- Accéder au document