Survey Observations of c-C2H4O and CH3CHO toward Massive Star-forming Regions

By M. Ikeda, M. Ohishi, A. Nummelin, J. Dickens, P. Bergman, Å. Hjalmarson, W. Irvine. 2001

139 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/106a6bac631769ce23ebeaf27adf3e99add2eaf7

How researchers see this paper

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In Astronomy and Astrophysics

1. Cecilia Ceccarelli
2. J. Jørgensen
3. E. V. van Dishoeck
4. Jonathan P. Williams
5. S. Bisschop
6. S. Bottinelli
7. France.
8. U. Hawaii

In Atmospheric Science

1. Cecilia Ceccarelli
2. E. V. van Dishoeck
3. Jonathan P. Williams
4. S. Bottinelli
5. S. Bisschop
6. Mark R. Morris
7. M. Requena-Torres
8. Jesús Martín-Pintado

In Spectroscopy

1. Cecilia Ceccarelli
2. Jonathan P. Williams
3. E. V. van Dishoeck
4. J. Jørgensen
5. S. Bottinelli
6. France.
7. Mark R. Morris
8. M. Requena-Torres

Citations in the corpus

• The Galactic Center: The Largest Oxygen-bearing Organic Molecule Repository (2007, background): “…observations of the aldehyde/alcohol pairs in hot cores have shown that the COM chemistry favors the reduced alcohols with respect to their corresponding aldehydes ( Ikeda et al. 2001; Hollis et al. 2002; Bisschop et al. 2007), i.e., the double bond between the C and the O must be easily broken.”
• Formation of ethylene glycol and other complex organic molecules in star-forming regions (2016, background): “…where saturated species, such as EG, are always more abundant than unsaturated species, such as GA (see Table 7); and in star-forming regions (e.g. Ikeda et al. 2001, Hollis et al. 2002, Bisschop et al. 2007) Therefore, there is evidence that chemistry favors saturated versus unsaturated species.”
• Testing grain-surface chemistry in massive hot-core regions (2007, background): “The existence of both ices and gas-phase molecules around the same high-mass protostars suggests that the envelopes have temperatures that range from >200 K in the inner region to as low as 10 K in the cold outer part (e.g., van der Tak et al. 2000; Gibb et al. 2000b; Ikeda et al. 2001).”
• Organic molecules in the Galactic center - Hot core chemistry without hot cores (2006, background): “For the comparison between the GC and hot cores associated to massive star formation we have selected the homogeneous data set by Ikeda et al. (2001) for several hot cores (W51, NGC6334f, G327.”
• Hot corinos in NGC 1333-IRAS4B and IRAS2A (2006, background): “Data are taken from Gibb et al. (2000a) and references therein, and from Ikeda et al. (2001).”