Mass Loss Geometry in Symbiotic Binaries

Details Mass Loss Geometry in Symbiotic Binaries Mass Loss Geometry in Symbiotic Binaries

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..265..221c&link_type=abstract

Post-AGB Objects as a Phase of Stellar Evolution, Proceedings of the Toruń Workshop held July 5-7, 2000. Edited by R. Szczerba a

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

I briefly revise the properties of the extended ionised nebulae around symbiotic stars. These are key objects in the discussion of the effects produced by a detached stellar companion on the AGB mass loss, of the outflows from accreting post--AGB stars, and of the mutual interaction of the slow and fast winds produced in these binary systems. The phenomenology is illustrated by new results on three of the best known symbiotics: He 2-104 Hen 2-104 (the Southern Crab), RX Pup and CH Cyg.

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