The composition of ices in comet C/1995 O1 (Hale-Bopp) from radio spectroscopy

By J. Crovisier, D. Bockelée-Morvan, P. Colom, N. Biver, D. Despois, D. Lis. 2004

184 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology

View Paper: https://www.semanticscholar.org/paper/117553a5d6385b2b0ba9ec388b9e3557ac62b876

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In Astronomy and Astrophysics

1. E. Herbst
2. Y. Aikawa
3. C. Walsh
4. R. Garrod
5. T. Millar
6. S. W. Weaver
7. H. Nomura
8. Japan.

In Ecology

1. Japan.
2. Usa

Citations in the corpus

• Complex organic molecules in protoplanetary disks (2013, background): “The radical-radical formation routes ofs-HCOOH,s-NH2CHO, and s-HOCH2CHO all rely on the formation ofs-HCO which, in turn, is formed mainly via the hydrogenation ofs-CO.”
• Cometary glycine detected in samples returned by Stardust (2009, methodology): “These upper limits correspond to ~0.3% glycine by mass in cometary ice, or 0.05% glycine by mass in cometary material with a dust-to-ice ratio of 5 (Crovisier et al. 2004).”
• The composition of cometary volatiles (2004, background): “Further work on archive millimeter spectra of Comet Hale-Bopp led to the identification of ethylene glycol (HOCH2CH2OH) (Crovisier et al., 2004b) with an abundance of 0.25% relative to water.”