Low energy observations of Cygnus X-2 by Ariel VI |
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Authors: | A. M. Cruise R. E. Cole J. L. Culhane J. Osborne J. Zarnecki |
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Affiliation: | Mullard Space Science Laboratory, Department of Physics and Astronomy, University College London, UK;Department of Space Research, University of Birmingham, UK |
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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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