Interpretation of the [ClIII] Lines in Gaseous Nebulae

Details Interpretation of the [ClIII] Lines in Gaseous Nebulae Interpretation of the [ClIII] Lines in Gaseous Nebulae

May 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970pnas...66....1a&link_type=abstract

Proceedings of the National Academy of Sciences of the United States of America, Volume 66, Issue 1, pp. 1-5

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9

Scientific paper

The intensity ratio of the green λ λ 5517 and 5537 lines of [ClIII] serves as an indicatrix of the electron density in many gaseous nebulae whose spectra can be observed with an image converter. Quantitative interpretation of the line ratio requires accurate values of the collisional strengths and transition probabilities. With improved values of these parameters we have revised electron densities for a number of nebulae; the results seem to be in good accord with those derived from other criteria.

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