Disks and planets around massive white dwarfs

M Livio, J E Pringle, K Wood

Research output: Contribution to journalArticlepeer-review

29 Citations (Scopus)

Abstract

We predict the existence of dusty disks and possibly CO planets around massive white dwarfs. We show that the thermal emission from these disks should be detectable in the infrared. The planets may also be detectable either by direct infrared imaging, spectroscopy, or using the pulsations of the white dwarfs.

Original languageEnglish
Pages (from-to)L37
Number of pages3
JournalAstrophysical Journal Letters
Volume632
Issue number1
DOIs
Publication statusPublished - 10 Oct 2005

Keywords

  • accretion, accretion disks
  • planetary systems
  • white dwarfs
  • SIZE DISTRIBUTION
  • COOL COMPANIONS
  • ACCRETION DISKS
  • RADIUS RELATION
  • STARS
  • EVOLUTION
  • ENERGY

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