The role of energetic processing on solid-phase chemistry in star forming regions
Date Issued
2015
Author(s)
•
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Kaňuchová, Z.
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Scirè, C.
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•
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Strazzulla, G.
Abstract
It is generally accepted that complex molecules observed in star forming regions are formed in the solid phase on icy grain mantles and are released to the gas-phase after desorption of icy mantles. Most of our knowledge on the physical and chemical properties of ices in star forming regions is based on the comparison between observations and laboratory experiments performed at low temperature (10-100 K). Here we present some recent laboratory experiments which show the formation of (complex) molecular species after ion bombardment of simple ices.
Coverage
Conditions and Impact of Star Formation: From Lab to Space
All editors
Simon, R.; Schaaf, R.; Stutzki, J.
Series
Volume
75-76
Start page
309
Conferenece
6th Zermatt ISM Symposium: Conditions and Impact of Star Formation: From Lab to Space
Conferenece place
Zermatt, Switzerland
Conferenece date
September 7-11, 2015
Issn Identifier
1633-4760
Ads BibCode
2015EAS....75..309P
Rights
open.access
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