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A Comparison of Radio-Frequency and Optical Studies of Selected Planetary Nebulae
Published online by Cambridge University Press: 25 April 2016
Extract
The thermal radio-frequency emission, Ev, per unit volume per unit frequency interval may be computed (e.g. from equations given by Oster) and compared with the volume emissivity E(Hβ) in the optical Hβ transition.
- Type
- Contributions
- Information
- Publications of the Astronomical Society of Australia , Volume 1 , Issue 6 , September 1969 , pp. 283 - 285
- Copyright
- Copyright © Astronomical Society of Australia 1969
References
2
Aller, L. H., ‘Gaseous Nebulae’, Chapman & Hall, London 1956; Seaton, M. J., Reports, Progess in Physics, 23, 313 (1960); Aller, L. H., and Liller, W., ‘Nebulae & Interstellar Matter’, Chap. 9, ed. Middlehurst, Barbara & Aller, L. H., University of Chicago Press, Chicago
1968.Google Scholar
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Clarke, Wm., Thesis, Univ. of California, Los Angeles, 1965, cf. p. 521 of ‘Nebulae & Interstellar Matter’, op. cit.Google Scholar
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Terzian, Y., I.A.U. symposium No. 34, ‘Planetary Nebulae’, ed. Osterbrock, D. and O’Dell, C. R., Reidel, Dordrecht-Holland
1968.Google Scholar
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See Kaler, J. B., Ap. J., 143, 722 (1966) and also series of papers entitled ‘Spectrophotometry Studies of Gaseous Nebulae’, ed. Czyzak, S. J., Kaler, J. B., Aller, L. H. and others in Ap. J.Google Scholar