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Spectrophotometry of 14 southern planetary nebulae

Published online by Cambridge University Press:  14 August 2015

L. H. Aller  and
D. J. Faulkner
L. H. Aller
Affiliation:
University of California, Los Angeles
D. J. Faulkner
Affiliation:
Mount Stromlo Observatory

Extract

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The theory of radiative and collisional processes in gaseous nebulae makes possible precise predictions of line and continuum intensities as functions of density, electron temperature, and degree of ionization of the emitting gases. It predicts, for example, the relative intensities of successive members of the Balmer series (Balmer decrement), and of corresponding transitions in the Balmer and Paschen series. Hence accurate line intensity measurements are not only of astrophysical interest; they also serve to assess the amount of space absorption.

Type
Section 1: The Galaxy
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 45 - 50
Copyright
Copyright © Australian Academy of Science 1964 

References

Aller, L. H. (1951).— Ap. J. 113: 125–40.Google Scholar
Code, A. (1960).—“Stars and Stellar Systems.” (General Ed. Kuiper, G. P..) vol. VI. pp. 50–87. (Univ. Chicago Press.)Google Scholar
Liller, W. (1957).—P. A. S. P. 69: 511–17.Google Scholar
Liller, W., and Aller, L. H. (1954).— Ap. J. 120: 48–57.Google Scholar
Menzel, D. H., Aller, L. H., and Hebb, M. H. (1941).— Ap. J. 93: 230–5.Google Scholar
Oke, J. B. (1960).— Ap. J. 131: 358–62.Google Scholar
Seaton, M. J. (1960).— Rep. Progr. Phys. (London) 23: 313–54.Google Scholar