The Dependence of H2CO and CH3OH Formation on the Temperature and Thickness of H2O-CO Ice during the Successive Hydrogenation of CO

By N. Watanabe, T. Shiraki, A. Kouchi. 2003

146 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/43d4b53d173569a653d2534cef7da1380bfeab40

How researchers see this paper

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

In Astronomy and Astrophysics

1. R. Garrod
2. E. Dishoeck
3. K. Oberg
4. H. Cuppen
5. H. Linnartz
6. S. Ioppolo
7. E. V. van Dishoeck
8. J. Jørgensen

In Atmospheric Science

1. R. Garrod
2. E. Dishoeck
3. H. Cuppen
4. K. Oberg
5. S. Ioppolo
6. E. V. van Dishoeck
7. H. Linnartz
8. J. Jørgensen

Citations in the corpus

• A COLD COMPLEX CHEMISTRY TOWARD THE LOW-MASS PROTOSTAR B1-b: EVIDENCE FOR COMPLEX MOLECULE PRODUCTION IN ICES (2010, background): “CO:CH3OH ice mixtures are probably common since CH3OH forms from hydrogenation of CO (e.g. Watanabe et al. 2003; Cuppen et al. 2009).”
• Photodesorption of ices I: CO, N₂, and CO₂ (2008, background): “The ices are subsequently processed by atom or light interactions to form more complex species (Tielens & Hagen 1982; Watanabe et al. 2003; Ioppolo et al. 2008).”
• Laboratory Evidence for Efficient Water Formation in Interstellar Ices (2008, background): “In addition, hydrogenation experiments on CO showed that the decreasing H coverage for increasing temperature results in lower effective rates (Watanabe et al. 2003, 2006; Linnartz et al. 2007; Cuppen et al. 2008).”
• Formation rates of complex organics in UV irradiated CH3OH-rich ices I: Experiments (2009, background): “Small molecules: H2, H2O, CH4, CO, O2, H2CO, H2O2 and CO2 H2 probably forms in the photolysis experiments, since CH2O is observed and thus H atoms must be produced in the ice (see below).”
• Hydrogenation reactions in interstellar CO ice analogues A combined experimental/theoretical approach (2009, background): “In a series of papers, these conflicting results were discussed (Hiraoka et al. 2002; Watanabe et al. 2003, 2004) and the prevailing discrepancy between results was proposed to be a consequence of different experimental conditions, most noticeable the adopted H-atom flux (Hidaka et al. 2004).”