XMM-Newton observations of AM CVn binaries

  • Ramsay, G.
  • Hakala, P.
  • Marsh, T.
  • Nelemans, G.A.
  • Steeghs, D.
  • Cropper, M.
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Publication date
January 2005
Publisher
EDP Sciences
ISSN
0004-6361
Citation count (estimate)
9

Abstract

Contains fulltext : 33048.pdf ( ) (Open Access) Contains fulltext : 33048.pdf (publisher's version ) (Open Access)We present the results of XMM-Newton observations of four AM CVn systems - AM CVn, CR Boo, HP Lib and GP Com. Their light curves show very different characteristics. The X-ray light curves show no coherent pulsations, suggesting the accreting white dwarfs have relatively low magnetic field strengths. Their spectra were best modelled using a multi-temperature emission model and a strong UV component. We find tha

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