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 …
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 …
Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it is difficult to observe from Earth. The Herschel Space Observatory provided …
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 …
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 …
AD Bosman, F Alarcón, EA Bergin… - The Astrophysical …, 2021 - iopscience.iop.org
The elemental composition of the gas and dust in a protoplanetary disk influences the compositions of the planets that form in it. We use the Molecules with ALMA at Planet …
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 …
Context. The total gas mass is one of the most fundamental properties of disks around young stars, because it controls their evolution and their potential to form planets. To measure disk …
N van der Marel - The European Physical Journal Plus, 2023 - epjplus.epj.org
Protoplanetary disks surrounding young stars are the birth place of planets. Of particular interest are the transition disks with large inner dust cavities of tens of au, hinting at the …