Properties of Cool Stellar Components in S-Type Symbiotic Stars

  • O. G. Taranova
  • B. F. Yudin
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 145)


In 1975 Webster and Allen (1975) divided all symbiotic stars into two groups-those in which the 1—4 M m continuum show only the presence of a cool star (type S),and those in which dust emission dominates (type D). With the exception of some of yellow symbiotic stars, the dust presence in others correlates with the spectral type of their cool components. That is why one can say that S-type symbiotics contain red giants with spectral type earlier than M6–M7.


coLour Index Spectral Type Asymptotic Branch Giant Cool Star Cool Component 
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

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • O. G. Taranova
    • 1
  • B. F. Yudin
    • 1
  1. 1.Sternberg State Astronomical InstituteMoscowUSSR

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