Zobrazeno 1 - 10
of 221
pro vyhledávání: '"François LIQUE"'
Publikováno v:
Frontiers in Chemistry, Vol 7 (2019)
Fine-structure populations and collision–induced energy transfer in atoms are of interest for many fields, from combustion to astrophysics. In particular, neutral carbon atoms are known to play a role in interstellar media, either as probes of phys
Externí odkaz:
https://doaj.org/article/218a312002af4983a37f08d04c50a1cf
Autor:
Floris F. S. van der Tak, François Lique, Alexandre Faure, John H. Black, Ewine F. van Dishoeck
Publikováno v:
Atoms, Vol 8, Iss 2, p 15 (2020)
The Leiden Atomic and Molecular Database (LAMDA) collects spectroscopic information and collisional rate coefficients for molecules, atoms, and ions of astrophysical and astrochemical interest. We describe the developments of the database since its i
Externí odkaz:
https://doaj.org/article/75e5ccde0bd44431b86cd525535c5d81
Publikováno v:
Journal of Physical Chemistry A
Journal of Physical Chemistry A, 2023, 127 (10), pp.2306-2313. ⟨10.1021/acs.jpca.2c08712⟩
The Journal of Physical Chemistry A, 127, 10, pp. 2306-2313
The Journal of Physical Chemistry A, 127, 2306-2313
Journal of Physical Chemistry A, 2023, 127 (10), pp.2306-2313. ⟨10.1021/acs.jpca.2c08712⟩
The Journal of Physical Chemistry A, 127, 10, pp. 2306-2313
The Journal of Physical Chemistry A, 127, 2306-2313
International audience; We report an experimental study of state-to-state inelastic scattering of NH (X 3 sigma-, N = 0, j = 1) radicals with He atoms. Using a crossed molecular beam apparatus that combines a Zeeman decelerator and velocity map imagi
Autor:
Ahmad Mortada, Sophie Carles, Sándor Demes, Baptiste Joalland, François Lique, Abdessamad Benidar, Panayotis Lavvas, Ludovic Biennier
Publikováno v:
ACS Earth and Space Chemistry
ACS Earth and Space Chemistry, 2022, 6 (5), pp.1227-1238. ⟨10.1021/acsearthspacechem.1c00347⟩
ACS Earth and Space Chemistry, 2022, 6 (5), pp.1227-1238. ⟨10.1021/acsearthspacechem.1c00347⟩
International audience; The photoionization of N2 plays a key role in initiating the formation of complex organic molecules in the nitrogen-rich atmosphere of Saturn’s largest moon, Titan. To date, only a handful of laboratory studies have explored
Autor:
Fabien Dumouchel, Ernesto Quintas-Sánchez, Christian Balança, Richard Dawes, François Lique, Nicole Feautrier
Publikováno v:
Journal of Chemical Physics
Journal of Chemical Physics, 2023, 158 (16), pp.164307. ⟨10.1063/5.0148119⟩
Journal of Chemical Physics, 2023, 158 (16), pp.164307. ⟨10.1063/5.0148119⟩
International audience; Interstellar anions play an important role in astrochemistry as being tracers of the physical and chemical conditions in cold molecular clouds and circumstellar gas. The local thermodynamic equilibrium is generally not fulfill
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::36af9d2f1fc6a688f841f480890e8a0d
https://hal.science/hal-04090181
https://hal.science/hal-04090181
Autor:
Marie Gueguen, François Lique
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 522 (4), pp.6251-6257. ⟨10.1093/mnras/stad1436⟩
Monthly Notices of the Royal Astronomical Society, 2023, 522 (4), pp.6251-6257. ⟨10.1093/mnras/stad1436⟩
The detection of the N+ ion in ionized interstellar regions, as well as its use as a tracer for atomic nitrogen (N) in interstellar media, makes it an interesting ion from the astrophysical point of view. Accurate determination of the N+ abundance in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd400f07791c85cec88cf59d81f3e297
https://hal.science/hal-04109532/file/50093749_File000008_1230227044.pdf
https://hal.science/hal-04109532/file/50093749_File000008_1230227044.pdf
Autor:
P. Hily-Blant, Sándor Demes, Claire Rist, Floris van der Tak, François Lique, Alexandre Faure
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, ⟨10.1093/mnras/stab3015⟩
Monthly Notices of the Royal Astronomical Society, 2022, 509 (1), pp.1252-1261. ⟨10.1093/mnras/stab3015⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2022, 509 (1), pp.1252-1261. ⟨10.1093/mnras/stab3015⟩
Monthly Notices of the Royal Astronomical Society, 509(1), 1252-1261. Oxford University Press
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, ⟨10.1093/mnras/stab3015⟩
Monthly Notices of the Royal Astronomical Society, 2022, 509 (1), pp.1252-1261. ⟨10.1093/mnras/stab3015⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2022, 509 (1), pp.1252-1261. ⟨10.1093/mnras/stab3015⟩
Monthly Notices of the Royal Astronomical Society, 509(1), 1252-1261. Oxford University Press
Free-access link :https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stab3015/6406505?guestAccessKey=80b41295-5352-4131-b205-23069ebc314cYu9hD1fx2MVcUv6Uxu7LQ==; International audience; The hydronium cation plays a crucial role in inter
Autor:
Francesca Tonolo, Cristina Puzzarini, Vincenzo Barone, Mattia Melosso, François Lique, Luca Bizzocchi
Publikováno v:
Proceedings of the 2022 International Symposium on Molecular Spectroscopy.
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Relaxation of the spin-orbit excited C+(2P3/2) ion by collisions with H2 is an important process in the interstellar medium. Previous calculations of rate coefficients for this process employed potential energies computed for only collinear and perpe
Rotational excitation of CO2 induced by He: New potential energy surface and scattering calculations
Publikováno v:
Journal of Chemical Physics
Journal of Chemical Physics, 2022, 156 (10), pp.104303. ⟨10.1063/5.0085094⟩
Journal of Chemical Physics, 2022, 156 (10), pp.104303. ⟨10.1063/5.0085094⟩
The CO2 molecule is of great interest for astrophysical studies since it can be found in a large variety of astrophysical media where it interacts with the dominant neutral species, such as He, H2, or H2O. The CO2–He collisional system was intensiv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::75e63ba5ac479e880a63510fbeb095d3
https://hal.science/hal-03632769
https://hal.science/hal-03632769