Helium Deficiency in Old Halo B Stars

Details Helium Deficiency in Old Halo B Stars Helium Deficiency in Old Halo B Stars

Mar 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.213..871g&link_type=abstract

Nature, Volume 213, Issue 5079, pp. 871-873 (1967).

Physics

60

Scientific paper

Calculations show that in old halo B stars most helium will have
diffused below the photosphere and therefore will not be detected
spectroscopically. This may account for the low abundances of helium
observed in these stars.

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