9 citations · 24 across the 5 of their papers we have counts for
5 papers
Simulation of proton radiolysis of H2O and O2 ices with the Nautilus code
Tian-Yu Tu, Valentine Wakelam, Jean-Christophe Loison +3
The radiolysis effect of cosmic rays (CRs) plays an important role in the chemistry in molecular clouds. CRs can dissociate the molecules on dust grains, producing reactive suprath…
Survey of (sub)mm water masers in low-mass star-forming regions
P. K. Humire, C. Goddi, G. N. Ortiz-León +2
Water masers are common in star-forming regions (SFRs), with the 22.235 GHz transition widely detected in both high- and low-mass protostars. In contrast, (sub)millimeter water mas…
Impact of the transport of magnetospheric electrons on the composition of the Triton atmosphere
B. Benne, B. Benmahi, M. Dobrijevic +5
Due to its inclined orbit and the complex geometry of the magnetic field of Neptune, Triton experiences a highly variable magnetic environment. As precipitation of magnetospheric e…
Chemical inventory of the envelope of the Class I protostar L1551 IRS 5
P. Marchand, A. Coutens, J. Scigliuto +5
Episodic accretion in protostars leads to luminosity outbursts that end up heating their surroundings. This rise in temperature pushes the snow lines back, enabling the desorption…
A photochemical model of Triton's atmosphere with an uncertainty propagation study
B. Benne, M. Dobrijevic, T. Cavalié +2
Triton is the largest satellite of Neptune and probably a Kuiper Belt Object that was captured by the planet. It has a tenuous nitrogen atmosphere similar to the one of Pluto and m…