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 …
The chemical composition of comets—emerging taxonomies and natal heritage
MJ Mumma, SB Charnley - Annual Review of Astronomy and …, 2011 - annualreviews.org
Cometary nuclei contain the least modified material from the formative epoch of our
planetary system, and their compositions reflect a range of processes experienced by …
planetary system, and their compositions reflect a range of processes experienced by …
An Ice Age JWST inventory of dense molecular cloud ices
MK McClure, WRM Rocha, KM Pontoppidan… - Nature …, 2023 - nature.com
Icy grain mantles are the main reservoir of the volatile elements that link chemical processes
in dark, interstellar clouds with the formation of planets and the composition of their …
in dark, interstellar clouds with the formation of planets and the composition of their …
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 …
Our astrochemical heritage
P Caselli, C Ceccarelli - The Astronomy and Astrophysics Review, 2012 - Springer
Our Sun and planetary system were born about 4.5 billion years ago. How did this happen,
and what is the nature of our heritage from these early times? This review tries to address …
and what is the nature of our heritage from these early times? This review tries to address …
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 …
Binding energies of interstellar molecules on crystalline and amorphous models of water ice by ab initio calculations
In the denser and colder (≤ 20 K) regions of the interstellar medium (ISM), near-infrared
observations have revealed the presence of submicron-sized dust grains covered by several …
observations have revealed the presence of submicron-sized dust grains covered by several …
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 …
Ice structures, patterns, and processes: A view across the icefields
From the frontiers of research on ice dynamics in its broadest sense, this review surveys the
structures of ice, the patterns or morphologies it may assume, and the physical and chemical …
structures of ice, the patterns or morphologies it may assume, and the physical and chemical …