Astrochemistry : recent successes and current challenges : proceedings of the 231st Symposium of the International Astronomical Union held in Pacific Grove, California, USA August 29 - September 2,…
By D. Lis, G. Blake, E. Herbst. 2005
164 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/1c33a7578b1cd45130e44474a6415a8ef1b65fa7
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Citations in the corpus
- Cometary glycine detected in samples returned by Stardust (2009, background): “Over 140 molecular species have been identified in the interstellar medium (ISM) by their rotational spectra (Lis et al. 2006), and more than two dozen organic molecules have been detected to date from spectroscopic observations of comets (Bockelee-Morvan et al. 2004).”
- Molecular Evolution and Star Formation: From Prestellar Cores to Protostellar Cores (2007, unknown): “Using molecular dynamics calculations, Kroes & Andersson (2006) showed that it is unlikely that this fraction is larger than 1%.”
- Formation rates of complex organics in UV irradiated CH3OH-rich ices I: Experiments (2009, background): “…most complex products is discussed by e.g. Hudson & Moore (2000) who investigated the production of complex molecules in CH3OH:H2O and CH3OH:CO ice mixtures both following UV irradiation and ion bombardment in a number of studies, most recently in Moore & Hudson (2005) and Hudson et al. (2005).”
- Experimental evidence for glycolaldehyde and ethylene glycol formation by surface hydrogenation of CO molecules under dense molecular cloud conditions (2015, background): “(8) Another formation route suggested later by Charnley & Rodgers (2005) is very similar but with altered sequences of H− and O−atom additions.”
- Simulation of the Formation and Morphology of Ice Mantles on Interstellar Grains (2007, background): “There is experimental and/or theoretical evidence that these reactions do indeed occur on cold surfaces (Kroes & Andersson 2006; Hiraoka et al. 1994; Tielens & Hagen 1982; Watanabe & Kouchi 2002).”
- Photodesorption of water ice - A molecular dynamics study (2008, methodology): “Photodesorption is also used to interpret the tentative detections of HDO and other gaseous species in the surface layers of protoplanetary disks (Willacy & Langer 2000; Dominik et al. 2005).”