activity
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.GAShow all

5 papers · 1 filter

astro-ph.GA2016★ 64 cited

Water delivery from cores to disks: deuteration as a probe of the prestellar inheritance of H2O

K. Furuya, M. N. Drozdovskaya, R. Visser +5

We investigate the delivery of regular and deuterated forms of water from prestellar cores to circumstellar disks. We adopt a semi-analytical axisymmetric two-dimensional collapsin…

astro-ph.GA2016★ 21 cited

On the Inference of the Cosmic Ray Ionization Rate from the HCO-to-DCO Abundance Ratio: The Effect of Nuclear Spin

Christopher N. Shingledecker, Jennifer B. Bergner, Romane Le Gal +3

The chemistry of dense interstellar regions was analyzed using a time-dependent gas-grain astrochemical simulation and a new chemical network that incorporates deuterated chemistry…

astro-ph.GA2016★ 49 cited

Chemical and physical characterization of collapsing low-mass prestellar dense cores

U. Hincelin, B. Commercon, V. Wakelam +3

The first hydrostatic core, also called the first Larson core, is one of the first steps in low-mass star formation, as predicted by theory. With recent and future high performance…

astro-ph.GA2015★ 87 cited

Water deuteration and ortho-to-para nuclear spin ratio of H2 in molecular clouds formed via the accumulation of HI gas

K. Furuya, Y. Aikawa, U. Hincelin +4

We investigate the water deuteration ratio and ortho-to-para nuclear spin ratio of H2 (OPR(H2)) during the formation and early evolution of a molecular cloud, following the scenari…

astro-ph.GA2012★ 94 cited

Elemental nitrogen partitioning in dense interstellar clouds

Julien Daranlot, Ugo Hincelin, Astrid Bergeat +4

Many chemical models of dense interstellar clouds predict that the majority of gas-phase elemental nitrogen should be present as N2, with an abundance approximately five orders of…