T
Thanja Lamberts
Researcher at Leiden University
Publications - 61
Citations - 1811
Thanja Lamberts is an academic researcher from Leiden University. The author has contributed to research in topics: Astrochemistry & Reaction rate constant. The author has an hindex of 22, co-authored 55 publications receiving 1406 citations. Previous affiliations of Thanja Lamberts include Radboud University Nijmegen & University of Stuttgart.
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Journal ArticleDOI
Grain Surface Models and Data for Astrochemistry
Herma M. Cuppen,Catherine Walsh,Catherine Walsh,Thanja Lamberts,Thanja Lamberts,D. Semenov,Robin T. Garrod,E. M. Penteado,Sergio Ioppolo +8 more
TL;DR: A broad consensus has been reached in the astrochemistry community on how to suitably treat gas-phase processes in models, and also how to present the necessary reaction data in databases; however, no such consensus has yet been reached for grain-surface processes.
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Experimental evidence for glycolaldehyde and ethylene glycol formation by surface hydrogenation of CO molecules under dense molecular cloud conditions
Gleb Fedoseev,Herma M. Cuppen,Sergio Ioppolo,Thanja Lamberts,Thanja Lamberts,Harold Linnartz +5 more
TL;DR: In this article, the formation of two molecules of astrobiological importance, glycolaldehyde(HC(O)CH2OH) andethyleneglycol(H2C(OH)CH 2OH) by surface hydrogenation of CO molecules, was investigated.
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The kinetic Monte Carlo method as a way to solve the master equation for interstellar grain chemistry.
TL;DR: The interstellar medium is far from empty; rather it contains large molecular clouds consisting of dust and gas, and many of the simple important molecules such as H2 and H2O and also several complex organic molecules are not formed in the gas phase, but rather on the grain surfaces themselves.
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Low-temperature surface formation of NH3 and HNCO: hydrogenation of nitrogen atoms in CO-rich interstellar ice analogues
Gleb Fedoseev,Sergio Ioppolo,Sergio Ioppolo,Dongfeng Zhao,Thanja Lamberts,Thanja Lamberts,Harold Linnartz +6 more
TL;DR: In this article, the formation routes of NH_3 and HNCO through non-energetic surface reactions in interstellar ice analogues under fully controlled laboratory conditions and at astrochemically relevant temperatures are investigated.
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Water formation at low temperatures by surface O2 hydrogenation III: Monte Carlo simulation
TL;DR: Using Continuous-Time Random-Walk Monte Carlo simulations to disentangle the different processes at play during hydrogenation of molecular oxygen, a set of 'best fit' parameters is presented and discussed for use in future astrochemical modeling.