Publication Abstracts

Greenstein et al. 1967

Greenstein, G.S., J.W. Truran, and A.G.W. Cameron, 1967: Helium deficiency in old Halo B stars. Nature, 213, 871-873, doi:10.1038/213871a0.

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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BibTeX Citation

  author={Greenstein, G. S. and Truran, J. W. and Cameron, A. G. W.},
  title={Helium deficiency in old Halo B stars},

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RIS Citation

ID  - gr08800u
AU  - Greenstein, G. S.
AU  - Truran, J. W.
AU  - Cameron, A. G. W.
PY  - 1967
TI  - Helium deficiency in old Halo B stars
JA  - Nature
VL  - 213
SP  - 871
EP  - 873
DO  - 10.1038/213871a0
ER  -

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