X-ray pulsations in the supersoft x-ray binary CAL 83

Jul, 2005
12 pages
Published in:
  • Astron.J. 131 (2006) 600-602
e-Print:

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Abstract: (arXiv)
X-ray data reveal that the supersoft X-ray binary CAL 83 exhibits 38.4 minute pulsations at some epochs. These X-ray variations are similar to those found in some novae and are likely to be caused by nonradial pulsations the white dwarf. This is the first detection of pulsations in a classical supersoft X-ray binary.
  • stars: individual (CAL 83)
  • stars: oscillations
  • X-rays: binaries
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