Untangling the formation of the cyclic carbon trioxide isomer in low temperature carbon dioxide ices

By C. Bennett, C. Jamieson, A. Mebel, Ralf I. Kaiser. 2004

161 citations recorded by the source corpus.

Subfields: Atmospheric Science, Atomic and Molecular Physics, and Optics, Inorganic Chemistry

View Paper: https://www.semanticscholar.org/paper/eae5c955bfc4fec5ab66fb0e5b1ee1516b45325a

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atmospheric Science

1. H. Linnartz
2. S. Ioppolo
3. H. Cuppen
4. E. V. van Dishoeck
5. Ralf I. Kaiser
6. C. Bennett
7. C. Romanzin
8. D. Jewitt

In Atomic and Molecular Physics, and Optics

1. E. V. van Dishoeck
2. H. Linnartz
3. S. Ioppolo
4. Ralf I. Kaiser
5. H. Cuppen
6. C. Bennett
7. M. Mottl
8. B. Glazer

In Inorganic Chemistry

1. Ralf I. Kaiser
2. C. Bennett
3. H. Linnartz
4. E. V. van Dishoeck

Citations in the corpus

• On the Formation of Glycolaldehyde (HCOCH2OH) and Methyl Formate (HCOOCH3) in Interstellar Ice Analogs (2007, methodology): “To calculate the column densities within our sample, a modified Lambert-Beers relationship is used (Bennett et al. 2004).”
• Temperature Dependence of the Formation of Hydrogen, Oxygen, and Hydrogen Peroxide in Electron-Irradiated Crystalline Water Ice (2006, background): “…is released via the electronic interaction potential leading to electronic excitation, vibrational excitation, bond ruptures, and ionization (Bennett et al. 2004; Jamieson et al. 2005; Kaiser 2002); therefore, electron irradiation experiments present the simplest way elucidate whether…”
• Water and astrobiology (2007, methodology): “Bennett et al. (2004) carried out experiments in a contamination-free ultrahigh vacuum (UHV) chamber (Fig.”
• A Combined Experimental and Theoretical Study on the Formation of the Amino Acid Glycine (NH2CH2COOH) and Its Isomer (CH3NHCOOH) in Extraterrestrial Ices (2005, background): “…absorption features of carbon dioxide at 3708 cm 1 (integral absorption coefficient A ¼ 1:4 ; 10 18 cm) and 3600 cm 1 (A ¼ 4:5 ;10 19 cm) and of methylamine at 1600 cm 1 (A ¼ 4:3 ;10 18 cm) and 1150 cm 1 (A ¼ 1:5 ;10 18 cm) and applied a modified Lambert-Beer relationship (Bennett et al. 2004).”
• Laboratory Evidence for Efficient Water Formation in Interstellar Ices (2008, methodology): “After fitting the infrared spectra with a straight baseline, the column density (molecules cm 2) of the newly formed species in the ice is calculated from the integrated intensity of the infrared bands using amodifiedLambertBeer equation (Bennett et al. 2004).”