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Christine Joblin

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Articles 45
Citations 165
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Recent Articles
1.
Bernard J, Martin S, Al-Mogeeth A, Joblin C, Ji M, Zettergren H, et al.
Phys Chem Chem Phys . 2024 Jul; 26(27):18571-18583. PMID: 38949429
The radiative cooling of naphthalene dimer cations, (CH) was studied experimentally through action spectroscopy using two different electrostatic ion-beam storage rings, DESIREE in Stockholm and Mini-Ring in Lyon. The spectral...
2.
Berne O, Habart E, Peeters E, Schroetter I, Canin A, Sidhu A, et al.
Science . 2024 Feb; 383(6686):988-992. PMID: 38422128
Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiation produces photodissociation regions (PDRs)...
3.
M Nair A, Leboucher H, Toucouere L, Zamith S, Joblin C, LHermite J, et al.
Phys Chem Chem Phys . 2024 Jan; 26(7):5947-5961. PMID: 38294026
Protonated mixed pyrene-water clusters, (Py)(HO)H, where = [1-3] and = [1-10], are generated using a cryogenic molecular cluster source. Subsequently, the mass-selected mixed clusters undergo controlled collisions with rare gases,...
4.
Zamith S, Kassem A, LHermite J, Joblin C, Cuny J
J Chem Phys . 2023 Nov; 159(18). PMID: 37955320
We report threshold collision induced dissociation experiments on protonated water clusters thermalized at low temperature for sizes n = 19-23. Fragmentation cross sections are recorded as a function of the...
5.
Berne O, Martin-Drumel M, Schroetter I, Goicoechea J, Jacovella U, Gans B, et al.
Nature . 2023 Jun; 621(7977):56-59. PMID: 37364766
Forty years ago, it was proposed that gas-phase organic chemistry in the interstellar medium can be initiated by the methyl cation CH (refs. ), but so far it has not...
6.
Garcia G, Dontot L, Rapacioli M, Spiegelman F, Brechignac P, Nahon L, et al.
Phys Chem Chem Phys . 2023 Feb; 25(6):4501-4510. PMID: 36722859
We present a combined experimental and theoretical study on the dissociative ionisation of clusters of pyrene. We measured the experimental appearance energies in the photon energy range 7.2-12.0 eV of...
7.
Banhatti S, Rap D, Simon A, Leboucher H, Wenzel G, Joblin C, et al.
Phys Chem Chem Phys . 2022 Nov; 24(44):27343-27354. PMID: 36326610
Polycyclic aromatic hydrocarbons (PAHs) are thought to be a major constituent of astrophysical environments, being the carriers of the ubiquitous aromatic infrared bands (AIBs) observed in the spectra of galactic...
8.
Vinitha M, Mundlapati V, Marciniak A, Carlos M, Sabbah H, Bonnamy A, et al.
J Phys Chem A . 2022 Aug; 126(33):5632-5646. PMID: 35951364
Polycyclic aromatic hydrocarbons are major species in astrophysical environments, and this motivates their study in samples of astrochemical interest such as meteorites and laboratory analogues of stardust. Molecular analyses of...
9.
Zamith S, Kassem A, LHermite J, Joblin C
J Phys Chem A . 2022 Jun; 126(23):3696-3707. PMID: 35670699
We report measurements of the attachment rates of water molecules onto mass-selected cationic pyrene clusters for size from = 4 to 13 pyrene units and for different collision energies. Comparison...
10.
Jenniskens P, Gabadirwe M, Yin Q, Proyer A, Moses O, Kohout T, et al.
Meteorit Planet Sci . 2021 Jul; 56(4):844-893. PMID: 34295141
The June 2, 2018, impact of asteroid 2018 LA over Botswana is only the second asteroid detected in space prior to impacting over land. Here, we report on the successful...