Gianfranco Vidali
Affiliations: | Physics | Syracuse University, Syracuse, NY, United States |
Area:
Astrophysics Physics, Physical ChemistryGoogle:
"Gianfranco Vidali"Mean distance: (not calculated yet)
Children
Sign in to add traineeJoseph E. Roser | grad student | 2004 | Syracuse |
Jiao He | grad student | 2014 | Syracuse |
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Publications
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Emtiaz SM, Toriello F, He J, et al. (2022) Infrared Spectroscopic Study of Methane Ice, Pure and in Mixtures with Polar (HO) and Nonpolar (N) Molecules. The Journal of Physical Chemistry. A |
Emtiaz SM, Toriello F, He J, et al. (2020) Infrared Spectroscopic Study of Solid Methane: Nuclear Spin Conversion of Stable and Metastable Phases. The Journal of Physical Chemistry. A |
He J, Clements AR, Emtiaz S, et al. (2019) The Effective Surface Area of Amorphous Solid Water Measured by the Infrared Absorption of Carbon Monoxide The Astrophysical Journal. 878: 94 |
Petucci J, Semone S, LeBlond C, et al. (2018) Formation of H on graphene using Eley-Rideal and Langmuir-Hinshelwood processes. The Journal of Chemical Physics. 149: 014702 |
He J, Emtiaz S, Boogert A, et al. (2018) The 12CO2 and 13CO2 Absorption Bands as Tracers of the Thermal History of Interstellar Icy Grain Mantles The Astrophysical Journal. 869: 41 |
He J, Emtiaz S, Vidali G. (2018) Measurements of Diffusion of Volatiles in Amorphous Solid Water: Application to Interstellar Medium Environments The Astrophysical Journal. 863: 156 |
He J, Emtiaz SM, Vidali G. (2017) Mechanism of Atomic Hydrogen Addition Reactions on np-ASW The Astrophysical Journal. 851: 104 |
He J, Emtiaz SM, Vidali G. (2017) Diffusion and Clustering of Carbon Dioxide on Non-porous Amorphous Solid Water The Astrophysical Journal. 837: 65 |
He J, Vidali G. (2017) Characterization of thin film CO2 ice through the infrared ν1 + ν3 combination mode Monthly Notices of the Royal Astronomical Society. 473: 860-866 |
Wakelam V, Bron E, Cazaux S, et al. (2017) H 2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations Molecular Astrophysics. 9: 1-36 |