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Bowen Resonance Fluorescence Lines of OIII in Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

C. R. O'Dell  and
C. O. Miller
C. R. O'Dell
Affiliation:
RICE UNIVERSITY P. O. Box 1892 Houston, Texas, USA
C. O. Miller
Affiliation:
RICE UNIVERSITY P. O. Box 1892 Houston, Texas, USA

Abstract

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New and published line intensities are used to test the role of the pumping of the Bowen Lines of O III by absorption of the O1 and O3 lines and population by Charge Exchange. Although general agreement is obtained, noticeable deviations from theory exist.

Type
III. Highlights on the Nebulae
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 191
Copyright
Copyright © Kluwer 1993 

References

Gargaud, I., McCarroll, R., & Opradolce, L.: 1989, A&A 208, 251 Google Scholar
Harrington, J. P.: 1972, ApJ 176, 127 CrossRefGoogle Scholar
Likkel, L. & Aller, L. H.: 1986, ApJ 301, 825 Google Scholar
O'Dell, C. R. & Miller, C. O.: 1992, ApJ 390, 219 Google Scholar
Sternberg, A., Dalgarno, A., & Roueff, E.: 1988, Comm. Ap. 13, 29 Google Scholar