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Propellers — A New Class of Interacting Binaries

Published online by Cambridge University Press:  25 May 2016

M. Mikołajewski ,
J. Mikołajewska  and
T. Tomov
M. Mikołajewski
Affiliation:
Institute of Astronomy, N. Copernicus University Chopina 12/18, PL-87100 Toruń, Poland
J. Mikołajewska
Affiliation:
Copernicus Astronomical Center Bartycka 18, PL-00716 Warsaw, Poland
T. Tomov
Affiliation:
National Astronomical Observatory Rozhen 4700 Smoljan, PB 136, Bulgaria

Abstract

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CH Cyg and MWC 560 are very peculiar symbiotic binaries consisting of an M giant and a white-dwarf companion. The systems have many features in common. In particular, both show occasional eruptions with sub-Eddington luminosity accompanied by flickering activity, and appearance of high-velocity jets. We present arguments that objects like CH Cyg and MWC 560 form a new subclass of interacting binaries distinguished by the presence of wind accreting magnetic white dwarfs.

Type
7 Cataclysmic Variables
Information
Symposium - International Astronomical Union , Volume 165: Compact Stars in Binaries , 1996 , pp. 451 - 456
Copyright
Copyright © Kluwer 1996 

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