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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.

Information

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

References

Doroshenko, V.T. et al. 1993, Inf. Bull. Var. Stars 4980.Google Scholar
Illarionov, A.F. & Sunyaev, R.A. 1975, A&A 39, 185.Google Scholar
Kolev, D. & Tomov, T. 1993, A&AS 100, 1.Google Scholar
Leedjärv, L., Mikołajewski, M. & Tomov, T. 1994, A&A 287, 543.Google Scholar
Lipunov, V.M. 1987, Ap&SS 132, 1.Google Scholar
Luthardt, R. 1991, Inf. Bull. Var. Stars 3563.Google Scholar
Michalitsianos, A.G. et al. 1991, ApJ 371, 761.Google Scholar
Michalitsianos, A.G. et al. 1993, ApJ 409, L53.CrossRefGoogle Scholar
Mikolajewska, J. & Kenyon, S.J. 1992, MNRAS 256, 177.CrossRefGoogle Scholar
Mikolajewska, J., Selvelli, P.L. & Hack, M. 1988, A&A 198, 150.Google Scholar
Mikołajewski, M. & Mikołajewska, J. 1994, MNRAS (submitted).Google Scholar
Mikołajewski, M., Mikołajewska, J. & Khudyakova, T.N. 1990a, A&A 235, 219.Google Scholar
Mikołajewski, M. et al. 1990b, Acta Astr. 40, 129.Google Scholar
Mikołajewski, M., Szczerba, R. & Tomov, T. 1988, in The Symbiotic Phenomenon , Mikołajewska, J. et al. (Eds.), Kluwer, p. 221.CrossRefGoogle Scholar
Mikołajewski, M., Tomov, T. & Mikołajewska, J. 1987, Ap&SS 131, 733.Google Scholar
Shore, S.N., Aufdenberg, J.P. & Michalitsianos, A.G. 1994, AJ 108, 671.CrossRefGoogle Scholar
Skopal, A., Mikołajewski, M. & Biernikowicz, R. 1989, Bull. Astr. Inst. Czechosl. 40, 433.Google Scholar
Solf, J. 1987, A&A 180, 207.Google Scholar
Taylor, A.R., Seaquist, E.R. & Kenyon, S.J. 1988, in The Symbiotic Phenomenon , Mikołajewska, J. et al. (Eds.), Kluwer, p. 231.Google Scholar
Taylor, A.R., Seaquist, E.R. & Mattei, J. 1985, Nat 359, 38.Google Scholar
Thakar, A. & Wing, R.F. 1992, BAAS 24, 801.Google Scholar
Tomov, T. et al. 1994, in Evolutionary links in the Zoo of interacting binaries , d'Antona, F. (Ed.), (in press).Google Scholar
Tomov, T. et al. 1990, Nat 346, 637.Google Scholar
Tomov, T. et al. 1992, MNRAS 258, 23.Google Scholar
Wachter, S. et al. 1994, in Interacting Binary Stars , Shafter, A.W. (Ed.), ASP Conference Series Vol. 56, p. 401.Google Scholar