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Low energy observations of Cygnus X-2 by Ariel VI
Authors:A. M. Cruise   R. E. Cole   J. L. Culhane   J. Osborne  J. Zarnecki
Affiliation:Mullard Space Science Laboratory, Department of Physics and Astronomy, University College London, UK;Department of Space Research, University of Birmingham, UK
Abstract:Ariel VI observations of Cygnus X-2 have revealed a rather flat spectrum between 0.1 and 1.5 keV with variable emission at low energy. Of the two conflicting interpretations of this object in terms of i) a distant high-luminosity (Lx 1038 ergs s−1) binary and ii) a nearby low-luminosity (Lx 1035 ergs s−1) degenerate dwarf system, our measurements support the latter.
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