The DOI matches its Crossref record; 97 of the 97 references it cites were found in a registry or an index.
Photochemistry and Astrochemistry: Photochemical Pathways to Interstellar Complex Organic Molecules
Open accessAbstract
The interstellar medium is characterized by a rich and diverse chemistry. Many of its complex organic molecules are proposed to form through radical chemistry in icy grain mantles. Radicals form readily when interstellar ices (composed of water and other volatiles) are exposed to UV photons and other sources of dissociative radiation, and if sufficiently mobile the radicals can react to form larger, more complex molecules. The resulting complex organic molecules (COMs) accompany star and planet formation and may eventually seed the origins of life on nascent planets. Experiments of increasing sophistication have demonstrated that known interstellar COMs as well as the prebiotically interesting amino acids can form through ice photochemistry. We review these experiments and discuss the qualitative and quantitative kinetic and mechanistic constraints they have provided. We finally compare the effects of UV radiation with those of three other potential sources of radical production and chemistry in interstellar ices: electrons, ions, and X-rays.
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Cites
Complex Organic Interstellar Molecules
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Protoplanetary Disks and Their Evolution
Williams, J. P., & Cieza, L. A. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102548 · Cited by 1,403
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Draine, B. T. (1978) · The Astrophysical Journal Supplement Series · doi:10.1086/190513 · Cited by 1,342
The Formation and Depletion of Molecules in Dense Interstellar Clouds
Herbst, E., & Klemperer, W. (1973) · The Astrophysical Journal · doi:10.1086/152436 · Cited by 1,087
Observations of the Icy Universe
Boogert, A. C. A., Gerakines, P. A., & Whittet, D. C. B. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122348 · Cited by 1,040
Cold Dark Clouds: The Initial Conditions for Star Formation
Bergin, E. A., & Tafalla, M. (2007) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.45.071206.100404 · Cited by 1,022
Complex Chemistry in Star‐forming Regions: An Expanded Gas‐Grain Warm‐up Chemical Model
Garrod, R. T., Weaver, S. L. W., & Herbst, E. (2008) · The Astrophysical Journal · doi:10.1086/588035 · Cited by 928
The Chemical Composition of Comets—Emerging Taxonomies and Natal Heritage
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Interstellar Ice: The Infrared Space Observatory Legacy
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Amino acids from ultraviolet irradiation of interstellar ice analogues
Muñoz Caro, G. M., Meierhenrich, U. J., Schutte, W. A., Barbier, B., Arcones Segovia, A., Rosenbauer, H., Thiemann, W. H.-P., Brack, A., & Greenberg, J. M. (2002) · Nature · doi:10.1038/416403a · Cited by 829
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Prebiotic Systems Chemistry: Complexity Overcoming Clutter
Islam, S., & Powner, M. W. (2017) · Chem · doi:10.1016/j.chempr.2017.03.001 · Cited by 154
Quantum Computing for Molecular Biology**
Baiardi, A., Christandl, M., & Reiher, M. (2023) · ChemBioChem · doi:10.1002/cbic.202300120 · Cited by 93
Metadata
- Authors
- Öberg, K. I.
- Venue
- Chemical Reviews
- Publisher
- American Chemical Society (ACS)
- Published
- 2016-04-21
- Volume
- 116
- Issue
- 17
- Pages
- 9631-9663
- ISSN
- 0009-2665 (ISSN-L)
- 1520-6890
- OpenAlex
- W2335865334
- Cited by
- 474
- References
- 97
- FWCI
- 2.89
- Type
- journal article
- Language
- en
- Open access
- green
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.