Using laboratory studies of CO-H2O ices to understand the non-detection of a 2152 cm-1 (4.647 μm) band in the spectra of interstellar ices

Helen J Fraser, M P Collings, John W Dever, M R S McCoustra

Research output: Contribution to journalArticlepeer-review

44 Citations (Scopus)


We present results from laboratory experiments on layered CO-H2O-ice systems, carried out from sub-monolayer to multilayer CO coverages, and review recent experimental data, as published by the authors. Under certain specific laboratory conditions the 2152 cm(-1) feature, associated with CO molecules adsorbed at dangling-OH bonds at the ice surface, is 'missing'. A detailed analysis is used to understand why the same feature is not detected in spectra of interstellar ices. We conclude that the dangling-OH sites do exist in interstellar ices but that the sites are blocked by another species. The astronomical implications of this deduction are discussed.

Original languageEnglish
Pages (from-to)59-68
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Issue number1
Publication statusPublished - 1 Sep 2004


Dive into the research topics of 'Using laboratory studies of CO-H<sub>2</sub>O ices to understand the non-detection of a 2152 cm<sup>-1</sup> (4.647 μm) band in the spectra of interstellar ices'. Together they form a unique fingerprint.

Cite this