Stellar Structure.

Details Stellar Structure. Stellar Structure.

Jun 1931

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1931natur.127r.894r&link_type=abstract

Nature, Volume 127, Issue 3215, pp. 894 (1931).

Physics

Scientific paper

BY an unaccountable slip, a numerical error crept into our recent communication1 concerning the nuclei of planetary nebulæ. With the assumed data for a typical nucleus, it is the superficial area which is 1/43 of the sun's. With mass equal to the sun, the mean density comes out 400 gm./cm.3, and with the probable mass 80 suns, as 32,000 gm./cm.3. This is still high enough to justify the classification of these stars with the white dwarfs; but degeneracy of the gas appears to be only beginning, rather than far advanced.

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