Transiting Disintegrating Planetary Debris around WD 1145+017
arXiv:1804.01997 · doi:10.1007/978-3-319-55333-7_37
Abstract
More than a decade after astronomers realized that disrupted planetary material likely pollutes the surfaces of many white dwarf stars, the discovery of transiting debris orbiting the white dwarf WD 1145+017 has opened the door to new explorations of this process. We describe the observational evidence for transiting planetary material and the current theoretical understanding (and in some cases lack thereof) of the phenomenon.
Invited review chapter. Accepted March 23, 2017 and published October 7, 2017 in the Handbook of Exoplanets. 15 pages, 10 figures
References in corpus (18)
- The frequency of planetary debris around young white dwarfs
- A gaseous metal disk around a white dwarf
- The Chemical Composition of an Extrasolar Minor Planet
- Formation of planetary debris discs around white dwarfs I: Tidal disruption of an extremely eccentric asteroid
- Six White Dwarfs with Circumstellar Silicates
- Drifting Asteroid Fragments Around WD 1145+017
- Explaining the variability of WD 1145+017 with simulations of asteroid tidal disruption
- Liberating exomoons in white dwarf planetary systems
- The Drop during Less than 300 days of a Dusty White Dwarf's Infrared Luminosity
- Spectroscopic Evolution of Disintegrating Planetesimals: Minutes to Months Variability in the Circumstellar Gas Associated with WD 1145+017
- WD 1145+017 Photometric Observations During 8 Months of High Activity
- Gray transits of WD 1145+017 over the visible band
- The puzzling source IGR J17361-4441 in NGC 6388: a possible planetary tidal disruption event
- Another one grinds the dust: Variability of the planetary debris disc at the white dwarf SDSS J104341.53+085558.2
- Simultaneous infrared and optical observations of the transiting debris cloud around WD 1145+017
- Mass and eccentricity constraints on the planetary debris orbiting the white dwarf WD 1145+017
- Rocky Planet Formation: Quick and Neat
- Dynamical mass and multiplicity constraints on co-orbital bodies around stars
Cited by in corpus (11)
- Planetary Systems Around White Dwarfs
- A dearth of small particles in the transiting material around the white dwarf WD 1145+017
- The lifetimes of planetary debris discs around white dwarfs
- Embedding planetesimals into white dwarf discs from large distances
- Chaotic rotation and evolution of asteroids and small planets in high-eccentricity orbits around white dwarfs
- The quest for planets around subdwarfs and white dwarfs from Kepler space telescope fields: Part I. Techniques and tests of the methods
- Can tidal evolution lead to close-in planetary bodies around white dwarfs II: volcanism and transits
- Optical Observations of star clusters NGC 1513 and NGC 4147; white dwarf WD1145+017 and band imaging of star forming region Sh2-61 with the 3.6 meter Devasthal Optical Telescope
- There's No Place Like Home (in Our Own Solar System): Searching for ET Near White Dwarfs
- Extrasolar enigmas: from disintegrating exoplanets to exoasteroids
- The Drake Equation at 60: Reconsidered and Abandoned