DARTOIS, E.; NOBLE, Jennifer; CASELLI, P.; FRASER, H.; JIMÉNEZ-SERRA, I.; MATÉ, B.; MCCLURE, M.; MELNICK, G.; PENDLETON, Y.; SHIMONISHI, T.; SMITH, Z.; STURM, J.; TAILLARD, A.; WAKELAM, V.; BOOGERT, A.; DROZDOVSKAYA, M.; ERKAL, J.; HARSONO, D.; HERRERO, V.; IOPPOLO, S.; LINNARTZ, H.; MCGUIRE, B.; PEROTTI, G.; QASIM, D.; ROCHA, W.

doi:10.1038/s41550-023-02155-x

Metadatos

Licencia de uso del documento

DARTOIS, E.
Centre National de la Recherche Scientifique [CNRS]
Université Paris-Saclay
Institut des Sciences Moléculaires d'Orsay [ISMO]

NOBLE, Jennifer
Physique des interactions ioniques et moléculaires [PIIM]
Centre National de la Recherche Scientifique [CNRS]

CASELLI, P.
Dipartimento di Chimica "Giacomo Ciamician"

Idioma

Article de revue

Este ítem está publicado en

Nature Astronomy. 2024-01-09, vol. 8, n° 3, p. 359-367

Nature Publishing Group

Resumen en inglés

Clouds of gas and dust in the Galaxy are nurseries in which stars and planetary systems are born. Cold dust grains grow icy mantles -by accretion, surface chemistry, and collision mechanisms -during their journey from the diffuse interstellar medium to protoplanetary disks. Our "Ice Age" JWST observations of the dense Chamaeleon I cloud reveal that this growth starts early, before the protostellar phase, significantly modifying the ice absorption band spectroscopic profiles. Spectral analysis confirms that the grains reach micron sizes, implying myriad changes in local microphysics, including mass transfer from small to large grains, reduction in the grain surface available for chemistry, and modification of the penetration and propagation of radiation fields. Deformation of the observed profiles complicates chemical abundance determination. Observing extensive icy growth in dense clouds quantitatively constrains the grain size evolution prior to star-and planet-formation.< Leer menos

Palabras clave en inglés

Astrophysical dust

Interstellar medium

Laboratory astrophysics

URI

https://oskar-bordeaux.fr/handle/20.500.12278/203480

DOI

http://dx.doi.org/10.1038/s41550-023-02155-x

Proyecto europeo

Linking chemistry and physics in the planet-forming zones of disks

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804