Hostname: page-component-77c89778f8-m42fx Total loading time: 0 Render date: 2024-07-17T07:16:01.138Z Has data issue: false hasContentIssue false
  • English
  • Français

Molecular Abundance Variations Among and Within Cold, Dark Molecular Clouds

Published online by Cambridge University Press:  07 August 2017

Masatoshi Ohishi ,
William M. Irvine  and
Norio Kaifu
Masatoshi Ohishi
Affiliation:
Nobeyama Radio Observatory, Nobeyama, Mimamimaki, Minamisaku, Nagano 384-13, Japan
William M. Irvine
Affiliation:
Five College Radio Astronomy Observatory, 619 Lederle GRC, University of Massachusetts, Amherst, MA 01003, U.S.A.
Norio Kaifu
Affiliation:
National Astronomical Observatory, 2-21-1, Osawa, Mitaka, Tokyo 181, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Keywords

Interstellar MoleculesMolecular AbundanceChemical Evolution
Type
Quiescent Clouds and Regions of Star Formation
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 171 - 177
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

Herbst, E. & Leung, C. M. (1989) ApJS, 69, 271.Google Scholar
Hirahara, Y. et al. (1991) submitted to ApJ.Google Scholar
Irvine, W. M., Ohishi, M. and Kaifu, N. (1991) Icarus, 91, 2.Google Scholar
Suzuki, H. et al. (1991) submitted to ApJ.Google Scholar
Swade, D. A. (1989) ApJS, 71, 219.CrossRefGoogle Scholar