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Recombination emission from CII-region around Be-Stars

  • S. P. Tarafdar
  • K. M. V. Apparao
Part of the Astrophysics and Space Science Library book series (ASSL, volume 163)

Abstract

Various physical processes proposed for the explanation of the flaring emissions of Hα and at 6578 Å in Be stars have been critically examined. The idea that the flaring occurs when X-ray emitting compact companion of Be-star produces the excess ionization of the shell material appears to give best agreement with observation.

Keywords

Equivalent Width Compact Object Will Emit Dielectronic Recombination Flare Emission 
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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References

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Copyright information

© Kluwer Academic Publishers 1990

Authors and Affiliations

  • S. P. Tarafdar
    • 1
  • K. M. V. Apparao
    • 1
  1. 1.Tata Institute of Fundamental ResearchBombayIndia

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