The IUE survey of W UMa type binaries

Details The IUE survey of W UMa type binaries The IUE survey of W UMa type binaries

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..351r&link_type=abstract

In ESA 3rd European IUE Conf. p 351-354 (SEE N83-11889 02-88)

Physics

Binary Stars, Flux (Rate), Stellar Spectra, Chromosphere, Data Reduction, Iue, Plasma Temperature, Resonance Lines, Stellar Coronas, Stellar Luminosity, Stellar Winds

Scientific paper

Homogeneous reductions of IUE low resolution observations of the brighter W UMa contact binaries were analyzed in terms of the transition region line fluxes. The fluxes, together with X-ray data, were used to study emission strength dependence on the temperature of the emitting plasma and on the period of stellar rotation. The contact binaries are found to have similar transition region line fluxes irrespective of the period. However, the fluxes are much below values expected from a direct extrapolation of the data for the detached binaries of longer periods.

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