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20112018
most citedOxygen depletion in dense molecular clouds: a clue to a low O2 abundance?

157 citations · 638 across the 10 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2018★ 36 cited

Multiple paths of deuterium fractionation in protoplanetary disks

Yuri Aikawa, Kenji Furuya, Ugo Hincelin +1

We investigate deuterium chemistry coupled with the nuclear spin-state chemistry of H and H in protoplanetary disks. Multiple paths of deuterium fractionation are found;…

astro-ph.SR2014★ 39 cited

A New and Simple Approach to Determine the Abundance of Hydrogen Molecules on Interstellar Ice Mantles

Ugo Hincelin, Qiang Chang, Eric Herbst

Water is usually the main component of ice mantles, which cover the cores of dust grains in cold portions of dense interstellar clouds. When molecular hydrogen is adsorbed onto an…

astro-ph.SR2014★ 38 cited

Water deuterium fractionation in the high-mass star-forming region G34.26+0.15 based on Herschel/HIFI data

Audrey Coutens, Charlotte Vastel, Ugo Hincelin +8

Understanding water deuterium fractionation is important for constraining the mechanisms of water formation in interstellar clouds. Observations of HDO and HO transitions…

astro-ph.SR2013★ 53 cited

Survival of interstellar molecules to prestellar dense core collapse and early phases of disk formation

Ugo Hincelin, Valentine Wakelam, Benoît Commerçon +2

An outstanding question of astrobiology is the link between the chemical composition of planets, comets, and other solar system bodies and the molecules formed in the interstellar…

astro-ph.SR2011★ 157 cited

Oxygen depletion in dense molecular clouds: a clue to a low O2 abundance?

U. Hincelin, V. Wakelam, F. Hersant +4

Context: Dark cloud chemical models usually predict large amounts of O2, often above observational limits. Aims: We investigate the reason for this discrepancy from a theoretical p…