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Fine Structure of Nebular Emission Lines

  • Published:1970-10 Issue:5266 Volume:228 Page:44-44
  • ISSN:0028-0836
  • Container-title:Nature
  • language:en
  • Short-container-title:Nature

Author:

MEABURN J.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Reference8 articles.

1. Aller, L. H., International Astrophysics Series, 3, Gaseous Nebulae (Chapman and Hall Ltd, London, 1954).

2. Courtès, G., Louise, R., and Monnet, G., Ann. d'Astrophys., 31, 493 (1968).

3. Kent, N. A., Tayler, L. B., and Pearson, H., Phys. Rev., 30, 266 (1927).

4. Lewis, G. N., and Spedding, F. H., Phys. Rev., 43, 964 (1933).

5. Spedding, F. H., Shane, C. D., and Grace, N. S., Phys. Rev., 44, 58 (1933).

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1. THE EVOLUTION OF THE KINEMATICS OF NEBULAR SHELLS IN PLANETARY NEBULAE IN THE MILKY WAY BULGE;The Astrophysical Journal;2010-05-21

2. Recombination line intensities for hydrogenic ions: The fine-structure components of HI and HeII;Astronomy and Astrophysics Supplement Series;1999-03

3. Echelle measurements of the electron temperature of the giant halo of the planetary nebula NGC 6543;Monthly Notices of the Royal Astronomical Society;1991-10-15

4. The physical conditions within the poly-polar nebula NGC 6302 - III;Monthly Notices of the Royal Astronomical Society;1982-07-01

5. The Electron Temperatures of the [O III] Zone of M42;Monthly Notices of the Royal Astronomical Society;1976-01-01
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