Electron temperatures and densities of planetary nebulae determined from the nebular hydrogen recombination spectrum and temperature and density variations-Reference-Cited by-同舟云学术

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Electron temperatures and densities of planetary nebulae determined from the nebular hydrogen recombination spectrum and temperature and density variations

Published:2004-07 Issue:3 Volume:351 Page:935-955
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Zhang Y.,Liu X.-W.,Wesson R.,Storey P. J.,Liu Y.,Danziger I. J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/351/3/935/3597084/351-3-935.pdf

Reference39 articles.

1. Improving Predictions for Helium Emission Lines

2. The Line Spectra of Helium in Gaseous Nebulae

3. Theoretical Continuous Spectra of Gaseous Nebulae

4. Far-infrared line observations of planetary nebulae. I - The forbidden O III spectrum

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