Jets in Symbiotic Binaries

Details Jets in Symbiotic Binaries Jets in Symbiotic Binaries

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cnoc.conf...34m&link_type=abstract

The Second National Conference on Astrophysics of Compact Objects, held in Bologna (Italy), September 19 - 21, 2001, p. 34

Astronomy and Astrophysics

Astrophysics

Scientific paper

Jets in symbiotic binaries (very hot and luminous compact companions accreting from the cool Giants/SuperGiants they are orbiting) have been for long considered very rear fenomena until the recent discoveries are rapidly increasing their frequency. The jets in three symbiotic binaries have been discovered by radio interferometry (R Aqr, CH Cyg, RS Oph), while we discovered in the optical the other three cases (MWC 560, Hen 3-1341, StHα 190). The properties of these jets are compared and their nature discussed in the framework of symbiotic binaries.

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