activity
20142019
most citedProduction of complex organic molecules: H-atom addition versus UV irradiation

77 citations · 217 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201944 cited

Formation of interstellar propanal and 1-propanol ice: a pathway involving solid-state CO hydrogenation

D. Qasim, G. Fedoseev, K. -J. Chuang +6

1-propanol (CH3CH2CH2OH) is a three carbon-bearing representative of primary linear alcohols that may have its origin in the cold dark cores in interstellar space. To test this, we…

astro-ph.SR201921 cited

Extension of the HCOOH and CO2 solid-state reaction network during the CO freeze-out stage: inclusion of H2CO

D. Qasim, T. Lamberts, J. He +5

Formic acid (HCOOH) and carbon dioxide (CO2) are simple species that have been detected in the interstellar medium. The solid-state formation pathways of these species under experi…

astro-ph.GA201918 cited

Alcohols on the rocks: solid-state formation in a H3CCCH + OH cocktail under dark cloud conditions

D. Qasim, G. Fedoseev, T. Lamberts +5

A number of recent experimental studies have shown that solid-state complex organic molecules (COMs) can form under conditions that are relevant to the CO freeze-out stage in dense…

astro-ph.GA201777 cited

Production of complex organic molecules: H-atom addition versus UV irradiation

K. -J. Chuang, G. Fedoseev, D. Qasim +3

Complex organic molecules (COMs) have been identified in different environments in star- forming regions. Laboratory studies show that COMs form in the solid state, on icy grains,…

astro-ph.GA201627 cited

Importance of tunneling in H-abstraction reactions by OH radicals: The case of CH4 + OH studied through isotope-substituted analogs

Thanja Lamberts, Gleb Fedoseev, Johannes Kästner +2

We present a combined experimental and theoretical study focussing on the quantum tunneling of atoms in the reaction between CH4 and OH. The importance of this reaction pathway is…

astro-ph.GA201430 cited

On the relevance of the H2 + O reaction pathway for the surface formation of interstellar water - A combined experimental and modeling study

Thanja Lamberts, Herma Cuppen, Gleb Fedoseev +3

The formation of interstellar water has been commonly accepted to occur on the surfaces of icy dust grains in dark molecular clouds at low temperatures (10-20 K), involving hydroge…