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.
|DOI (Digital Object Identifier) Link:||https://doi.org/10.1039/b518088k|
|Google Scholar:||Look up in Google Scholar|
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.
|Item Type:||Journal Article|
|Academic Unit/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)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Astrid Peterkin|
|Date Deposited:||08 May 2008|
|Last Modified:||29 Nov 2016 16:55|
|Share this page:|