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Jets from symbiotic stars

Published online by Cambridge University Press:  04 August 2017

M. Kafatos ,
A. Cassatella ,
A.G. Michalitsianos ,
L. Piro  and
R. Viotti
M. Kafatos
Affiliation:
1. George Mason University, Dept. Physics, Fairfax, VA, USA
A. Cassatella
Affiliation:
2. IUE Observatory, ESA, Madrid, Spain
A.G. Michalitsianos
Affiliation:
3. Laboratory for Astronomy and Solar Physics, NASA-GSFC, Greenbelt, MD, USA
L. Piro
Affiliation:
4. Instituto TESRE, CNR, Bologna, Italy
R. Viotti
Affiliation:
5. Instituto Astrofisica Spaziale, CNR, Frascati, Italy

Abstract

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R Aquarii is the closest symbiotic variable that shows extended emission with multiple jet components. A number of other symbiotics also show jet activity and this phenomenon may be common, particularly among D-type symbiotics.

Type
Symbiotic Stars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 491 - 492
Copyright
Copyright © Reidel 1987 

References

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