Photoelectric Spectrophotometry of Planetary Nebulæ

Details Photoelectric Spectrophotometry of Planetary Nebulæ Photoelectric Spectrophotometry of Planetary Nebulæ

Mar 1954

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1954natur.173..589m&link_type=abstract

Nature, Volume 173, Issue 4404, pp. 589-590 (1954).

Physics

9

Scientific paper

THE electron temperature of a planetary nebula can be determined from
the relative intensities of the N1 and N2 lines of
[OIII] at λλ5,007, 4,959, and the `auroral' type
transition at λ4,363, provided the target areas for collisional
excitation are known1.

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