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Astrophysics and Space Science

, Volume 78, Issue 2, pp 503–504 | Cite as

Intrinsic polarization variations of the symbiotic star R Aqr and the single-star hypothesis

  • J. Svatoš
  • M. Šolc
Letters to the Editor

Abstract

Due to similarity of the intrinsic polarization changes near phase 0.8 and due to other similar physical features observed both in o Ceti and R Aqr it is suggested that the activity in R Aqr system is caused by a flaring region on a single star.

Keywords

Flare Physical Feature Polarization Variation Polarization Change Single Star 
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.

References

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Copyright information

© D. Reidel Publishing Co 1981

Authors and Affiliations

  • J. Svatoš
    • 1
  • M. Šolc
    • 1
  1. 1.Dept. of Astronomy and AstrophysicsCharles UniversityPragueCzechslovakia

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