activity
20142021
most citedProduction of complex organic molecules: H-atom addition versus UV irradiation

77 citations · 149 across the 4 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA20262 cited

In situ characterization of volatile and refractory hydrocarbons produced by UV photolysis of interstellar CH ice

P. Samarth, G. Fedoseev, M. Bulak +5

Acetylene (CH) is commonly observed in star-forming regions, young stellar objects, and the Solar System. Laboratory and theoretical studies have linked this simplest alkyn…

astro-ph.GA202115 cited

Methoxymethanol Formation Starting from CO-Hydrogenation

Jiao He, Mart Simons, Gleb Fedoseev +7

Methoxymethanol (CH3OCH2OH, MM) has been identified through gas-phase signatures in both high- and low-mass star-forming regions. This molecule is expected to form upon hydrogen ad…

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…