[HTML][HTML] Grain surface models and data for astrochemistry
HM Cuppen, C Walsh, T Lamberts, D Semenov… - Space Science …, 2017 - Springer
The cross-disciplinary field of astrochemistry exists to understand the formation, destruction,
and survival of molecules in astrophysical environments. Molecules in space are …
and survival of molecules in astrophysical environments. Molecules in space are …
Surface processes on interstellar amorphous solid water: Adsorption, diffusion, tunneling reactions, and nuclear-spin conversion
T Hama, N Watanabe - Chemical reviews, 2013 - ACS Publications
Since we intend to review experimental and theoretical studies of physicochemical
processes occurring on cosmic dust grains in very cold regions in space, we start with a brief …
processes occurring on cosmic dust grains in very cold regions in space, we start with a brief …
Thermal desorption of interstellar ices: A review on the controlling parameters and their implications from snowlines to chemical complexity
M Minissale, Y Aikawa, E Bergin, M Bertin… - ACS Earth and Space …, 2022 - ACS Publications
The evolution of star-forming regions and their thermal balance are strongly influenced by
their chemical composition, which, in turn, is determined by the physicochemical processes …
their chemical composition, which, in turn, is determined by the physicochemical processes …
Early Planet Formation in Embedded Disks (eDisk). II. Limited Dust Settling and Prominent Snow Surfaces in the Edge-on Class I Disk IRAS 04302+ 2247
While dust disks around optically visible, Class II protostars are found to be vertically thin,
when and how dust settles to the midplane are unclear. As part of the Atacama Large …
when and how dust settles to the midplane are unclear. As part of the Atacama Large …
Direct mapping of the temperature and velocity gradients in discs-Imaging the vertical CO snow line around IM Lupi
Accurate measurements of the physical structure of protoplanetary discs are critical inputs
for planet formation models. These constraints are traditionally established via complex …
for planet formation models. These constraints are traditionally established via complex …
Binding energies: New values and impact on the efficiency of chemical desorption
Recent laboratory measurements have confirmed that chemical desorption (desorption of
products due to exothermic surface reactions) can be an efficient process. The impact of …
products due to exothermic surface reactions) can be an efficient process. The impact of …
[HTML][HTML] Dust as interstellar catalyst-I. Quantifying the chemical desorption process
Context. The presence of dust in the interstellar medium has profound consequences on the
chemical composition of regions where stars are forming. Recent observations show that …
chemical composition of regions where stars are forming. Recent observations show that …
Temperature structures of embedded disks: young disks in Taurus are warm
MLR Van't Hoff, D Harsono, JJ Tobin… - The Astrophysical …, 2020 - iopscience.iop.org
The chemical composition of gas and ice in disks around young stars sets the bulk
composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still …
composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still …
Early Planet Formation in Embedded Disks (eDisk). III. A First High-resolution View of Submillimeter Continuum and Molecular Line Emission toward the Class 0 …
Studying the physical and chemical conditions of young embedded disks is crucial to
constrain the initial conditions for planet formation. Here we present Atacama Large …
constrain the initial conditions for planet formation. Here we present Atacama Large …
Experimental evidence for glycolaldehyde and ethylene glycol formation by surface hydrogenation of CO molecules under dense molecular cloud conditions
G Fedoseev, HM Cuppen, S Ioppolo… - Monthly Notices of …, 2015 - academic.oup.com
This study focuses on the formation of two molecules of astrobiological importance–
glycolaldehyde (HC (O) CH2OH) and ethylene glycol (H2C (OH) CH2OH)–by surface …
glycolaldehyde (HC (O) CH2OH) and ethylene glycol (H2C (OH) CH2OH)–by surface …