Titre :

Thermal Desorption of Interstellar Ices: A Review on the Controlling Parameters and Their Implications from Snowlines to Chemical Complexity

Auteur(s) :

Minissale, Marco [Auteur correspondant]
Physique des interactions ioniques et moléculaires [PIIM]
Aikawa, Yuri [Auteur]
Department of Astronomy [Tokyo]
Bergin, Edwin [Auteur]
Bertin, Mathieu [Auteur]
Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères = Laboratory for Studies of Radiation and Matter in Astrophysics and Atmospheres [LERMA]
Brown, Wendy [Auteur]
Cazaux, Stephanie [Auteur]
Faculty of Aerospace Engineering [Delft]
Charnley, Steven [Auteur]
GSFC Solar System Exploration Division
Coutens, Audrey [Auteur]
Institut de recherche en astrophysique et planétologie [IRAP]
Cuppen, Herma [Auteur]
Institute for Molecules and Materials [Nijmegen]
Guzman, Victoria [Auteur]
Joint ALMA Observatory [JAO]
Linnartz, Harold [Auteur]
Mccoustra, Martin [Auteur]
Rimola, Albert [Auteur]
Departament de Química [Barcelona] [UAB]
Schrauwen, Johanna G.M. [Auteur]
Institute for Molecules and Materials [Nijmegen]
Toubin, Celine [Auteur]
Physico-Chimie Moléculaire Théorique [PCMT]
Ugliengo, Piero [Auteur]
Watanabe, Naoki [Auteur]
Institute of Low Temperature Science [Sapporo]
Wakelam, Valentine [Auteur]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Dulieu, Francois [Auteur]
LERMA Cergy [LERMA]

Titre de la revue :

ACS Earth and Space Chemistry

Pagination :

597-630

Éditeur :

ACS

Date de publication :

2022-03-17

ISSN :

2472-3452

Discipline(s) HAL :

Chimie/Chimie théorique et/ou physique
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]

Résumé en anglais : [en]

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 that govern the transition between the ...
Lire la suite >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 that govern the transition between the gas phase and the solid state, specifically icy dust grains (e.g., particle adsorption and desorption). Gas–grain and grain–gas transitions as well as formation and sublimation of interstellar ices are thus essential elements of understanding astrophysical observations of cold environments (e.g., prestellar cores) where unexpected amounts of a large variety of chemical species have been observed in the gas phase. Adsorbed atoms and molecules also undergo chemical reactions that are not efficient in the gas phase. Therefore, the parametrization of the physical properties of atoms and molecules interacting with dust grain particles is clearly a key aspect to interpret astronomical observations and to build realistic and predictive astrochemical models. In this consensus evaluation, we focus on parameters controlling the thermal desorption of ices and how these determine pathways toward molecular complexity and define the location of snowlines, which ultimately influence the planet formation process. We review different crucial aspects of desorption parameters both from a theoretical and experimental points of view. We critically assess the desorption parameters (the binding energies, Eb, and the pre-exponential factor, ν) commonly used in the astrochemical community for astrophysically relevant species and provide tables with recommended values. The aim of these tables is to provide a coherent set of critically assessed desorption parameters for common use in future work. In addition, we show that a nontrivial determination of the pre-exponential factor ν using transition state theory can affect the binding energy value. The primary focus is on pure ices, but we also discuss the desorption behavior of mixed, that is, astronomically more realistic, ices. This allows discussion of segregation effects. Finally, we conclude this work by discussing the limitations of theoretical and experimental approaches currently used to determine the desorption properties with suggestions for future improvements.Lire moins >

Langue :

Anglais

Vulgarisation :

Non

Projet ANR :

L'évolution chimique des proto-étoiles: de la phase profondément enfouie au disque protoplanétaire

Collections :

• Laboratoire de Physique des Lasers, Atomes et Molécules (PhLAM) - UMR 8523

Source :

Harvested from HAL