Computer Science
Scientific paper
Aug 1963
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1963natur.199..580g&link_type=abstract
Nature, Volume 199, Issue 4893, pp. 580-581 (1963).
Computer Science
21
Scientific paper
THE central stars of planetary nebulæ have effective temperatures1-3, Ts, ranging from 3 × 104 ° K to about 2.5 × 105 ° K. Such stars may therefore be much hotter than the hottest main sequence stars which have temperatures of about 4 × 104 ° K. To obtain a better understanding of the nature of very hot stars, a number of non-grey model atmospheres have been computed.
Gebbie Katharine B.
Seaton M. J.
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