Six White Dwarfs with Circumstellar Silicates
arXiv:0811.1740 · doi:10.1088/0004-6256/137/2/3191
Abstract
Spitzer Space Telescope spectra reveal 10 micron silicate emission from circumstellar dust orbiting six externally-polluted white dwarfs. Micron-size glasses with an olivine stoichiometry can account for the distinctively broad wings that extend to 12 microns; these particles likely are produced by tidal-disruption of asteroids. The absence of infrared PAH features is consistent with a scenario where extrasolar rocky planets are assembled from carbon-poor solids.
21 pages, 7 figures, AJ, in press
References in corpus (13)
- A gaseous metal disk around a white dwarf
- Transience of hot dust around sun-like stars
- The Chemical Composition of an Extrasolar Minor Planet
- Pollution of single white dwarfs by accretion of many small asteroids
- The shape and composition of interstellar silicate grains
- Externally-polluted white dwarfs with dust disks
- Debris Disks Around White Dwarfs: The DAZ Connection
- Carbon Deficiency in Externally-Polluted White Dwarfs: Evidence for Accretion of Asteroids
- The accretion-diffusion scenario for metals in cool white dwarfs
- SDSSJ104341.53+085558.2: A second white dwarf with a gaseous debris disc
- Infrared Emission from the Dusty Disk Orbiting GD 362, An Externally-Polluted White Dwarf
- Warm dust in the terrestrial planet zone of a sun-like Pleiad: collisions between planetary embryos?
- Circumstellar Dust Created by Terrestrial Planet Formation in HD 113766