Astrochemistry: From Molecular Clouds to Planetary Systems

By Y. Minh, E. Dishoeck. 2000

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Molecular Evolution in Collapsing Prestellar Cores (2001, unknown): “Bergin & Langer (1997) (See also Bergin 2000), on the other hand, have investigated molecular evolution in a prestellar core extensively.”
Molecular Evolution and Star Formation: From Prestellar Cores to Protostellar Cores (2007, background): “The observation of ices towards the low-mass protostar Elias 29 is summarized in Ehrenfreund & Shutte (2000); the abundances of CO, CO2, CH3OH and CH4 relative to water ice are 5.6 %, 22 %, < 4 %, and < 1.6 %, respectively.”
The Gas-Phase Formation of Methyl Formate in Hot Molecular Cores (2004, background): “Among the injected species are formaldehyde and methanol, for which grain-surface syntheses from CO have some basis in laboratory studies (Hiraoka et al. 2000; Watanabe & Kouchi 2002).”
Molecular Evolution in Collapsing Prestellar Cores. III. Contraction of a Bonnor-Ebert Sphere (2004, background): “With this convention, Table 1 summarizes ice compositions observed towards the field star Elias 16, the low-mass protostar Elias 29, and the high-mass protostars NGC 7538 IRS9, GL 7009S and W33A (Ehrenfreund & Shutte 2000; Gibb et al. 2000).”