White Dwarfs pp 337-338 | Cite as

The Search for Planets Around Pulsating White Dwarf Stars

  • F. Mullally
  • A. Mukadam
  • D. E. Winget
  • R. E. Nather
  • S. O. Kepler
Chapter
Part of the NATO Science Series book series (NAII, volume 105)

Abstract

We introduce a new technique to search for extra-solar planets with a different sensitivity from other methods, using the pulsations of white dwarf stars as intrinsic clocks. We will search for the effects of reflex orbital motion in changing light travel times and accelerations caused by any planets orbiting these stars. Our technique is sensitive to planets in the range 2-20 AU.

Keywords

Sine Argos 

References

  1. Kepler, S. O., et al 2000, ApJ, 534, L185ADSCrossRefGoogle Scholar
  2. Kepler, S. O., et al 1991, ApJ, 378, L45ADSCrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 2003

Authors and Affiliations

  • F. Mullally
    • 1
  • A. Mukadam
    • 1
  • D. E. Winget
    • 1
  • R. E. Nather
    • 1
  • S. O. Kepler
    • 2
  1. 1.Department of AstronomyUniversity of Texas at AustinUSA
  2. 2.Instituto de FísicaUniversidade Federal do Rio Grande do SulPorto AlegreBrazil

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