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Fabien Borget

Researcher at Aix-Marseille University

Publications -  40
Citations -  1460

Fabien Borget is an academic researcher from Aix-Marseille University. The author has contributed to research in topics: Astrochemistry & Interstellar ice. The author has an hindex of 20, co-authored 39 publications receiving 1300 citations. Previous affiliations of Fabien Borget include Clausthal University of Technology & University of Oldenburg.

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Hydrogenation of solid hydrogen cyanide HCN and methanimine CH2NH at low temperature

TL;DR: In this paper, the authors investigated the hydrogenation reaction network of hydrogen cyanide HCN and methanimine CH2 NH ices in an ultra-high vacuum experiment.
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Tentative identification of urea and formamide in ISO-SWS infrared spectra of interstellar ices

TL;DR: In this paper, a comparison of the infrared spectra of the photolysis products with spectra recorded from the protostellar source NGC 7538 IRS9 shows that the "unexplained" 1700 cm(-1) feature can be attributed to the contribution of several species H2CO (formaldehyde), HCONH2 (formamide) and H2NCONH2(urea) mixed with H2O as the main contributor.
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Thermal reactions in interstellar ice: A step towards molecular complexity in the interstellar medium

TL;DR: In this article, a list of purely thermal reactions involving electronically stable reactants to complement existing grain chemistry networks is provided, and the kinetic parameters of the reactions are given when available.
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Scientific rationale for Uranus and Neptune in situ explorations

TL;DR: In this article, the authors describe the main scientific goals to be addressed by a future in situ exploration of an ice giant, and a strawman ice-giant probe payload is described, with data returned to Earth using a Carrier Relay Spacecraft as a relay station.
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Formation of neutral methylcarbamic acid (CH3NHCOOH) and methylammonium methylcarbamate [CH3NH3+][CH3NHCO2-] at low temperature.

TL;DR: It is shown that amines can react at low temperature in interstellar ices rich in carbon dioxide which are a privileged place of complex molecules formation, before being later released into "hot core" regions.