Using cold plasma to investigate the mechanisms involved in cosmic dust formation: role of the C/O ratio and metals.
astrochemistry
dust
methods: laboratory
plasmas
stars: AGB and post-AGB
Journal
Proceedings of the International Astronomical Union. International Astronomical Union
ISSN: 1743-9221
Titre abrégé: Proc Int Astron Union
Pays: England
ID NLM: 101725418
Informations de publication
Date de publication:
Apr 2019
Apr 2019
Historique:
entrez:
19
10
2020
pubmed:
1
4
2019
medline:
1
4
2019
Statut:
ppublish
Résumé
Using a cold plasma reactor in which we inject an organosilicon molecular precursor, we investigate chemical mechanisms that can be involved in dust formation in evolved stars. By injecting metal atoms into the gas-phase, we investigate the role of metals on dust composition. We show the formation of composite particles made of pure metal (silver) nanoparticles embedded in an organosilicon dust. We study the impact of oxygen and show that it can inhibit dust formation, likely through the destruction of nucleation seeds.
Identifiants
pubmed: 33072172
doi: 10.1017/S1743921319008457
pmc: PMC7116203
mid: EMS92592
doi:
Types de publication
Journal Article
Langues
eng
Pagination
397-300Subventions
Organisme : European Research Council
ID : 610256
Pays : International