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 a.s an effect of chemical evolution.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Herbst, E. & Leung, C. M. (1989) ApJS, 69, 271.
Hirahara, Y. et al. (1991) submitted to ApJ.
Irvine, W. M., Ohishi, M. and Kaifu, N. (1991) Icarus, 91, 2.
Suzuki, H. et al. (1991) submitted to ApJ.
Swade, D. A. (1989) ApJS, 11, 219.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1992 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Ohishi, M., Irvine, W.M., Kaifu, N. (1992). Molecular Abundance Variations Among and Within Cold, Dark Molecular Clouds. In: Singh, P.D. (eds) Astrochemistry of Cosmic Phenomena. International Astronomical Union, vol 150. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2761-5_39
Download citation
DOI: https://doi.org/10.1007/978-94-011-2761-5_39
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-1825-5
Online ISBN: 978-94-011-2761-5
eBook Packages: Springer Book Archive