most citedFirst detection of triply-deuterated methanol

261 citations · 261 across the 2 of their papers we have counts for

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astro-ph2009101 cited

Cold CO in circumstellar disks: On the effects of photodesorption and vertical mixing

F. Hersant, V. Wakelam, A. Dutrey +2

Aims. We attempt to understand the presence of gas phase CO below its freezing temperature in circumstellar disks. We study two promising mechanisms to explain this phenomenon: tur…

astro-ph20085 cited

Time-dependent models of dense PDRs with complex molecules

O. Morata, E. Herbst

We present a study of the chemistry of a dense photon-dominated region (PDR) using a time-dependent chemical model. Our major interest is to study the spatial distribution of compl…

astro-ph2008115 cited

Modeling the Lukewarm Corino Phase - is L1527 unique?

George E. Hassel, Eric Herbst, Robin T. Garrod

Sakai et al. have observed long-chain unsaturated hydrocarbons and cyanopolyynes in the low-mass star-forming region L1527, and have attributed this result to a gas-phase ion-molec…

astro-ph2008913 cited

Complex Chemistry in Star-Forming Regions: An Expanded Gas-Grain Warm-up Chemical Model

Robin T. Garrod, Susanna L. Widicus Weaver, Eric Herbst

Gas-phase processes were long thought to be the key formation mechanisms for complex organic molecules in star-forming regions. However, recent experimental and theoretical evidenc…

astro-ph2007243 cited

Molecular Evolution and Star Formation: From Prestellar Cores to Protostellar Cores

Yuri Aikawa, Valentine Wakelam, Robin T. Garrod +1

We investigate molecular evolution in a star-forming core that is initially a hydrostatic starless core and collapses to form a low-mass protostar. The results of a one-dimensional…

astro-ph200793 cited

Chemistry in Protoplanetary Disks: A Sensitivity Analysis

A. I. Vasyunin, D. Semenov, Th. Henning +3

We study how uncertainties in the rate coefficients of chemical reactions in the RATE06 database affect abundances and column densities of key molecules in protoplanetary disks. We…