Astrophysics and Space Science

, Volume 6, Issue 1, pp 118–130 | Cite as

The helium-rich stars of early spectral type

  • Ann S. Dinger


The properties of the known helium-rich stars of early type are reviewed and the elemental abundances are analyzed. Current evolutionary theories of mixing and mass loss may explain the origin of these stars.


Mass Loss Evolutionary Theory Elemental Abundance Spectral Type Early Type 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© D. Reidel Publishing Company 1970

Authors and Affiliations

  • Ann S. Dinger
    • 1
  1. 1.Lindheimer Astronomical Research CenterNorthwestern UniversityEvanstonUSA

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