UPPER LIMITS FOR THE ETHYL-CYANIDE ABUNDANCES IN TMC-1 AND L134N - CHEMICAL IMPLICATIONS
Journal or Book Title
ASTROPHYSICS AND SPACE SCIENCE
We have sought interstellar ethyl-cyanide via its 202–101 transition towards two cold, dark clouds and report upper limits of the total column densities of 3×1012cm–2 and 2×1012cm–2 for TMC-1 and L134N, respectively. We also observed the 202–101 transition of vinyl cyanide previously identified in TMC-1 by Matthews and Sears (1983b). The detection of vinyl cyanide and the non-detection of ethyl cyanide in TMC-1 are consistent with gas phase ion-molecule chemical models, and there is thus no necessity of invoking grain surface synthesis for vinyl cyanide in cold clouds.
MINH, YC and Irvine, William M., "UPPER LIMITS FOR THE ETHYL-CYANIDE ABUNDANCES IN TMC-1 AND L134N - CHEMICAL IMPLICATIONS" (1991). ASTROPHYSICS AND SPACE SCIENCE. 243.
This document is currently not available here.