Hostname: page-component-745bb68f8f-lrblm Total loading time: 0 Render date: 2025-01-08T14:47:58.822Z Has data issue: false hasContentIssue false
  • English
  • Français

UV-Visible and Near IR Absorption Characteristics of Interstellar PAHS. I. C10H8+

Published online by Cambridge University Press:  07 August 2017

F. Salama  and
L. J. Allamandola
F. Salama
Affiliation:
NASA-Ames Research Center. Space Science Division, MS: 245-6 Moffett Field, CA 94035, U.S.A
L. J. Allamandola
Affiliation:
NASA-Ames Research Center. Space Science Division, MS: 245-6 Moffett Field, CA 94035, U.S.A

Abstract

An abstract is not available for this content so a preview has been provided. As you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Basic Studies
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 25 - 26
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

1 Salama, F. and Allamandola, L. J. (1991) ‘Electronic absorption spectroscopy of matrix -isolated polycyclic aromatic hydrocarbon cations. I. The naphthalene cation (C10H8 +)’, J. Chem. Phys. 94 (11), 6964–6977.CrossRefGoogle Scholar
2 Salama, F. and Allamandola, L. J. (1991) ‘The role of matrix material and CCl4 (electron acceptor) on the ionization mechanisms of matrix-isolated naphthalene’, J. Chem. Phys. (in press, Oct. 15 edition).CrossRefGoogle Scholar