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 language | English |
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Pages (from-to) | L37 |
Number of pages | 3 |
Journal | Astrophysical Journal Letters |
Volume | 632 |
Issue number | 1 |
DOIs | |
Publication status | Published - 10 Oct 2005 |
Keywords
- accretion, accretion disks
- planetary systems
- white dwarfs
- SIZE DISTRIBUTION
- COOL COMPANIONS
- ACCRETION DISKS
- RADIUS RELATION
- STARS
- EVOLUTION
- ENERGY