The latest table of molecular abundances in the cold, dark clouds TMC-1 and L134N is presented. Molecular abundance variations between TMC-1 and L134N, those within TMC-1 and L134N, and those among 49 dark cloud cores surveyed by Suzuki et al. (1991) are interpreted as an effect of chemical evolution.
CITATION STYLE
Ohishi, M., Irvine, W. M., & Kaifu, N. (1992). Molecular Abundance Variations Among and Within Cold, Dark Molecular Clouds. Symposium - International Astronomical Union, 150, 171–177. https://doi.org/10.1017/s0074180900089944
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