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Photochemistry and astrochemistry: Photochemical pathways to interstellar complex organic molecules
KI Öberg - Chemical reviews, 2016 - ACS Publications
The interstellar medium is characterized by a rich and diverse chemistry. Many of its
complex organic molecules are proposed to form through radical chemistry in icy grain …
complex organic molecules are proposed to form through radical chemistry in icy grain …
Prebiotic astrochemistry and the formation of molecules of astrobiological interest in interstellar clouds and protostellar disks
Despite the generally hostile nature of the environments involved, chemistry does occur in
space. Molecules are seen in environments that span a wide range of physical and chemical …
space. Molecules are seen in environments that span a wide range of physical and chemical …
LIDA: the Leiden ice database for astrochemistry
Context. High-quality vibrational spectra of solid-phase molecules in ice mixtures and for
temperatures of astrophysical relevance are needed to interpret infrared observations …
temperatures of astrophysical relevance are needed to interpret infrared observations …
Abiotic formation of alkylsulfonic acids in interstellar analog ices and implications for their detection on Ryugu
For the last century, the source of sulfur in Earth's very first organisms has remained a
fundamental, unsolved enigma. While sulfates and their organic derivatives with sulfur in the …
fundamental, unsolved enigma. While sulfates and their organic derivatives with sulfur in the …
Sulfur ice astrochemistry: a review of laboratory studies
Sulfur is the tenth most abundant element in the universe and is known to play a significant
role in biological systems. Accordingly, in recent years there has been increased interest in …
role in biological systems. Accordingly, in recent years there has been increased interest in …
Chemical evolution of CO2 ices under processing by ionizing radiation: Characterization of nonobserved species and chemical equilibrium phase with the …
Astrophysical ices are being exposed to ionizing radiation in space environments, which
trigger new reactions and desorption processes. In the lab, such processing by radiation has …
trigger new reactions and desorption processes. In the lab, such processing by radiation has …
Map** the evolution of pure CO2 ices irradiated by ions, UV, and electrons using the upgraded PROCODA code (employing an effective rate constant ordering by …
Chemical reactions and desorption processes are being triggered by incoming ionizing
radiation over astrophysical ices in cold space environments. The quantification of these …
radiation over astrophysical ices in cold space environments. The quantification of these …
Energetic electron irradiations of amorphous and crystalline sulphur-bearing astrochemical ices
Laboratory experiments have confirmed that the radiolytic decay rate of astrochemical ice
analogues is dependent upon the solid phase of the target ice, with some crystalline …
analogues is dependent upon the solid phase of the target ice, with some crystalline …
VIZSLA—Versatile ice zigzag sublimation setup for laboratory astrochemistry
In this article, a new multi-functional high-vacuum astrophysical ice setup, VIZSLA (Versatile
Ice Zigzag Sublimation Setup for Laboratory Astrochemistry), is introduced. The instrument …
Ice Zigzag Sublimation Setup for Laboratory Astrochemistry), is introduced. The instrument …
Characterization of acetonitrile ice irradiated by X-rays employing the procoda code – I. Effective rate constants and abundances at chemical equilibrium
In this work, the chemical evolution of pure acetonitrile ice at 13 K irradiated with broad-band
soft X-rays (from 6 eV to 2 keV) is determined by using a computational methodology …
soft X-rays (from 6 eV to 2 keV) is determined by using a computational methodology …