Copy the page URI to the clipboard
Mason, Nigel J.; Dawes, Anita; Holtom, Philip D.; Mukerji, Robin J.; Davis, Michael P.; Sivaraman, Bhalamurugan; Kaiser, Ralf I.; Hoffmann, Soren V. and Shaw, David A.
(2006).
DOI: https://doi.org/10.1039/b518088k
URL: http://www.rsc.org/publishing/journals/FD/article....
Abstract
In order to understand much of the chemistry that underpins astronomical phenomena (e.g. star and planet formation) it is essential to probe the physico-chemistry of ice surfaces under astronomical conditions. The physical properties and chemical reactivity of such icy surfaces depends upon its morphology. Thus it is necessary to explore how the morphology of astrochemical ices is influenced by their local environment (e.g. temperature and pressure) and the mechanisms by which they are processed. In this paper we report the results of a series of experiments to explore the morphology of a variety of molecular ices using VUV spectroscopy. Spectral signatures are found that may allow the morphology of such ices to be identified.
Viewing alternatives
Metrics
Public Attention
Altmetrics from AltmetricNumber of Citations
Citations from DimensionsItem Actions
Export
About
- Item ORO ID
- 10686
- Item Type
- Journal Item
- ISSN
- 1359-6640
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Faculty of Arts and Social Sciences (FASS) - Research Group
- Physics
- Depositing User
- Astrid Peterkin