Abstract
EXOSAT observations of the contact binary VW Cephei on 19th March 1984 are presented. The L1-telescope with CMA+thick Lexan filter was used. The observations cover one orbital revolution showing an asymmetrical X-ray light curve. This can be modelled by an active neck, connecting the two stars, and with enhanced coronal regions on the primary star. Nearly simultaneous IUE observations are also presented. The observations form a part of the program to observe contact binaries with EXOSAT.
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References
Binnendijk L 1970, Vistas in Astronomy 12, 217.
Cruddace R G, Dupree A K 1984, Astrophys. J. 277, 263.
Dupree A 1981, in R M Bonnet and A K Dupree (eds.), Solar Phenomena in Stars and Stellar Systems, D. Reidel Publ. Co. p. 407.
Eaton J A 1983, Astrophys. J. 268, 800.
Hazlehurst J, Meyer-Hofmeister E 1973, Astron. Astrophys. 24, 379.
Linsky J L 1983, in J O Stenflo (ed.), Solar and Stellar Magnetic Fields: Origins and Coronal Effects, D. Reidel Publ. Co. p. 313.
Mochnacki S W 1981, Astrophys. J. 245, 650.
Linnell A P 1982, Astrophys. J. 50, 85. (Suppl.)
Rahunen T 1981, Astron. Astrophys. 102, 81.
Rahunen T, Vilhu O 1982, in Z Kopal and J Rahe (eds.), Binary and Multiple Stars as Tracers of Stellar Evolution, D. Reidel Publ. Co. p. 289.
Rucinski S M 1973, Acta Astronomica 23, 79.
Rucinski S M, Vilhu O 1983, Mon. Not. R. astr. Soc. 202, 1221.
Smith R C 1984, (preprint)
van't Veer F 1979, Astron. Astrophys. 80, 287.
Vilhu O 1981, Astrophys. Space Sci. 78, 401.
Vilhu O 1982, Astron. Astrophys. 109, 17.
Vilhu O 1984, Astron. Astrophys. 133, 117.
Webbink R F 1977, Astrophys. J. 215, 851.
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Vilhu, O., Heise, J. EXOSAT observations of the contact binary VW Cephei. Space Sci Rev 40, 55–62 (1985). https://doi.org/10.1007/BF00212866
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DOI: https://doi.org/10.1007/BF00212866