Astrochemistry and compositions of planetary systems
KI Öberg, EA Bergin - Physics Reports, 2021 - Elsevier
Planets form and obtain their compositions in disks of gas and dust around young stars. The
chemical compositions of these planet-forming disks regulate all aspects of planetary …
chemical compositions of these planet-forming disks regulate all aspects of planetary …
Astrochemistry during the formation of stars
JK Jørgensen, A Belloche… - Annual Review of …, 2020 - annualreviews.org
Star-forming regions show a rich and varied chemistry, including the presence of complex
organic molecules—in both the cold gas distributed on large scales and the hot regions …
organic molecules—in both the cold gas distributed on large scales and the hot regions …
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 …
Formation of complex organic molecules in hot molecular cores through nondiffusive grain-surface and ice-mantle chemistry
A new, more comprehensive model of gas–grain chemistry in hot molecular cores is
presented, in which nondiffusive reaction processes on dust-grain surfaces and in ice …
presented, in which nondiffusive reaction processes on dust-grain surfaces and in ice …
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 …
[HTML][HTML] H2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations
Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …
A three-phase chemical model of hot cores: the formation of glycine
RT Garrod - The Astrophysical Journal, 2013 - iopscience.iop.org
ABSTRACT A new chemical model is presented that simulates fully coupled gas-phase,
grain-surface, and bulk-ice chemistry in hot cores. Glycine (NH 2 CH 2 COOH), the simplest …
grain-surface, and bulk-ice chemistry in hot cores. Glycine (NH 2 CH 2 COOH), the simplest …
Interstellar water chemistry: from laboratory to observations
Water is a fundamental molecule in the universe. On Earth, water exists in all three phases:
gas, liquid, and solid (ice). Liquid water facilitates many chemical reactions as a solvent …
gas, liquid, and solid (ice). Liquid water facilitates many chemical reactions as a solvent …
Gas and grain chemical composition in cold cores as predicted by the Nautilus three-phase model
We present an extended version of the two-phase gas–grain code nautilus to the three-
phase modelling of gas and grain chemistry of cold cores. In this model, both the mantle and …
phase modelling of gas and grain chemistry of cold cores. In this model, both the mantle and …
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 …