Astrophysical Estimates of Ionisation Potentials of Iron, Yttrium, and Lanthanum

Details Astrophysical Estimates of Ionisation Potentials of Iron, Yttrium, and Lanthanum Astrophysical Estimates of Ionisation Potentials of Iron, Yttrium, and Lanthanum

Jun 1928

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1928natur.121..906d&link_type=abstract

Nature, Volume 121, Issue 3058, pp. 906 (1928).

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THE work of Saha, Fowler, and Milne has shown how the intensities of ionised lines in stellar spectra are dependent upon temperature, pressure, ionisation, and excitation potentials. By studying the changes in intensity of a line from stars of one spectral class to another, astrophysical estimates have been made of the ionisation potentials of certain of the elements by several investigators.

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