Issue |
A&A
Volume 668, December 2022
|
|
---|---|---|
Article Number | A76 | |
Number of page(s) | 10 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202244506 | |
Published online | 08 December 2022 |
Ammonia, carbon dioxide, and the non-detection of the 2152 cm−1 CO band
1
Max Planck Institute for Astronomy,
Königstuhl 17,
69117
Heidelberg, Germany
e-mail: he@mpia.de
2
Physics Department, Syracuse University,
Syracuse, NY
13244, USA
3
Institute for Astronomy, University of Hawai’i at Manoa,
2680 Woodlawn Drive,
Honolulu, HI
968221839, USA
Received:
15
July
2022
Accepted:
10
October
2022
Context. CO is one of the most abundant ice components on interstellar dust grains. When it is mixed with amorphous solid water (ASW) or located on its surface, an absorption band of CO at 2152 cm−1 is always present in laboratory measurements. This spectral feature is attributed to the interaction of CO with dangling-OH bonds (dOH) in ASW. However, this band is absent in observational spectra of interstellar ices. This raises the question whether CO forms a relatively pure layer on top of ASW or is in close contact with ASW, but not via dangling bonds.
Aims. We aim to determine whether the incorporation of NH3 or CO2 into ASW blocks the dOH and therefore reduces the 2152 cm−1 band.
Methods. We performed laboratory experiments to simulate the layered structure of the ice mantle, that is, we grew CO ice on top of 1) pure ASW, 2) NH3:H2O=10:100 mixed ice, and 3) CO2:H2O=20:100 mixed ice. Infrared spectra were measured to quantify the strength of the 2152 cm−1 band. In addition, a second set of experiments were performed to determine how the incorporation of NH3 into ASW affects the dOH band.
Results. We found that annealing the ice reduces the 2152 cm−1 band and that NH3 blocks the dOH on ASW surface and therefore reduces the 2152 cm−1 band more effectively than CO2. We suggest that this difference between NH3 and CO2 can be ascribed to the polarity of the guest molecule (NH3 is a polar species, whereas CO2 is apolar). The polarity implies that the formation of an H-bond between the N atom of ammonia and the dOH is a barrier-less reaction. We also determined the pore surface area of the ice mixtures as a function of the annealing temperature, and found that the nondetection of 2152 cm−1 band does not necessarily exclude the possibility of a porous ice mantle.
Key words: astrochemistry / molecular processes / infrared: ISM / solid state: volatile / methods: laboratory: solid state / ISM: molecules
Note to the reader: The following sentence, inserted in the Abstract during the language editing process, was incorrectly published in the final version: "a title should be crisp and newspaper-style, and direct questions are to be avoided in scientific writing. Please rephrase your title and take this into account. Your running title may be a good place to start." This extra sentence has been removed from the Abstract on 5 January 2023.
© J. He et al. 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe-to-Open model.
Open Access funding provided by Max Planck Society.
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