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IUE-spectra of the four interacting binary white dwarf stars: AM CVn,PG 1346+082, V803 Cen,AND GP com. A comparative study
Authors:A M Ulla  J -E Solheim
Institution:(1) Institute of Mathematical and Physical Sciences, University of Tromsø, Tromsø, Norway
Abstract:This project is part of a world wide cooperation aimed at investigating properties of white dwarf stars to determine their constitution and evolution. The project is based on two recent developments:-The first is the discovery, of pulsational instabilities in some white dwarf stars, giving rise to non-radial pulsations which can be observed as flux modulations with low amplitude.-The second is to study the mass transfer between interacting binary white dwarf stars, which transports processed material from the interior of the donating star to the accretor. We present a study of four interacting binary white dwarf systems based on IUE spectra.Paper presented at the 11th European Regional Astronomical Meetings of the IAU on lsquoNew Windows to the Universersquo, held 3–8 July, 1989, Tenerife Canary Islands, Spain.
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