Copy the page URI to the clipboard
Mason, Nigel J.; Nair, Binukumar; Jheeta, Sohan and Szymańska, Ewelina
(2014).
DOI: https://doi.org/10.1039/C4FD00004H
Abstract
The commissioning of the ALMA array and the next generation of space telescopes heralds the dawn of a new age of Astronomy, in which the role of chemistry in the interstellar medium and in star and planet formation may be quantified. A vital part of these studies will be to determine the molecular complexity in these seemingly hostile regions and explore how molecules are synthesised and survive. The current hypothesis is that many of these species are formed within the ice mantles on interstellar dust grains with irradiation by UV light or cosmic rays stimulating chemical reactions. However, such irradiation releases many secondary electrons which may themselves induce chemistry. In this article we discuss the potential role of such electron induced chemistry and demonstrate, through some simple experiments, the rich molecular synthesis that this may lead to.
Viewing alternatives
Download history
Metrics
Public Attention
Altmetrics from AltmetricNumber of Citations
Citations from DimensionsItem Actions
Export
About
- Item ORO ID
- 40359
- Item Type
- Journal Item
- ISSN
- 1359-6640
- Extra Information
- This article is part of themed collection: Astrochemistry of Dust, Ice and Gas
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
- Physics
- Copyright Holders
- © 2014 The Royal Society of Chemistry
- Depositing User
- Ewelina Szymanska-Skolimowska