Abstract
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.
Cite
CITATION STYLE
APA
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
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free