UV-photoprocessing of interstellar ice analogs: New infrared spectroscopic results

By G. M. M. Caro, W. Schutte. 2003

181 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/d20ae71563a9a4947778385129a0086d3b7cda83

How researchers see this paper

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In Astronomy and Astrophysics

1. E. Dishoeck
2. R. Garrod
3. K. Oberg
4. E. V. van Dishoeck
5. H. Linnartz
6. J. Jørgensen
7. P. Caselli
8. Cecilia Ceccarelli

In Atomic and Molecular Physics, and Optics

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

In Spectroscopy

1. E. Dishoeck
2. R. Garrod
3. K. Oberg
4. E. V. van Dishoeck
5. H. Linnartz
6. J. Jørgensen
7. Cecilia Ceccarelli
8. P. Caselli

Citations in the corpus

• Formation rates of complex organics in UV irradiated CH3OH-rich ices I: Experiments (2009, unknown): “In the CH3OH photochemistry experiments, the ice films are irradiatedt normal or 45◦ inci- dence with UV light from a broadband hydrogen microwave-discharge lamp, which peaks around Ly α at 121 nm and covers 115–170 nm or 7–10.5 eV (Muñoz Caro & Schutte 2003).”
• Testing grain-surface chemistry in massive hot-core regions (2007, background): “Alternatively, both OCN− and NH2CHO can form in ices due to energetic processes such as UV-irradiation (van Broekhuizen et al. 2004; Muñoz Caro & Schutte 2003; Allamandola et al. 1999).”
• Photodesorption of ices I: CO, N₂, and CO₂ (2008, methodology): “The ice films are irradiated at normal or 45◦ incidence with UV light from a broadband hydrogen microwave discharge lamp, which peaks around Ly α at 121 nm and covers 115–170 nm or 7–10.5 eV (Muñoz Caro & Schutte 2003).”
• PHOTODESORPTION OF ICES. II. H2O AND D2O (2008, background): “The ice films are irradiated at normal or 45◦ incidence with UV light from a broadband hydrogen microwave discharge lamp, which peaks around Ly α at 121 nm and covers 115–170 nm or 7–10.5 eV (Muñoz Caro & Schutte 2003).”
• NON-RACEMIC AMINO ACID PRODUCTION BY ULTRAVIOLET IRRADIATION OF ACHIRAL INTERSTELLAR ICE ANALOGS WITH CIRCULARLY POLARIZED LIGHT (2011, background): “Among these organics, the detection of up to 16 different amino acids has been reported in one experiment including achiral (glycine, sarcosine, β-alanine) and chiral amino acids (alanine, serine, aspartic acid, etc.; Muñoz Caro et al. 2002), and confirmed in several other similar experiments (Bern”