Spitzer planet limits around the pulsating white dwarf GD66

Fergal Mullally, William T. Reach, Steven Degennaro, Adam S. Burrows

Research output: Contribution to journalArticle

20 Scopus citations

Abstract

We present infrared observations in search of a planet around the white dwarf, GD66. Time-series photometry of GD66 shows a variation in the arrival time of stellar pulsations consistent with the presence of a planet with mass ≥2.4M J. Any such planet is too close to the star to be resolved, but the planet's light can be directly detected as an excess flux at 4.5μm. We observed GD66 with the two shorter wavelength channels of the Infrared Array Camera on Spitzer but did not find strong evidence of a companion, placing an upper limit of 5-7M J on the mass of the companion, assuming an age of 1.2-1.7 Gyr.

Original languageEnglish (US)
Pages (from-to)327-331
Number of pages5
JournalAstrophysical Journal
Volume694
Issue number1
DOIs
StatePublished - 2009

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Infrared: stars
  • Planetary systems
  • Stars: oscillations
  • White dwarfs

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