Constraints on the circumstellar dust around KIC 8462852
arXiv:1512.03693 · doi:10.1093/mnrasl/slw008
Abstract
We present millimetre (SMA) and sub-millimetre (SCUBA-2) continuum observations of the peculiar star KIC 8462852 which displayed several deep and aperiodic dips in brightness during the Kepler mission. Our observations are approximately confusion-limited at 850 m and are the deepest millimetre and sub-millimetre photometry of the star that has yet been carried out. No significant emission is detected towards KIC 8462852. We determine upper limits for dust between a few 10 M and 10 M for regions identified as the most likely to host occluding dust clumps and a total overall dust budget of 7.7 M within a radius of 200 AU. Such low limits for the inner system make the catastrophic planetary disruption hypothesis unlikely. Integrating over the Kepler lightcurve we determine that at least 10 M of dust is required to cause the observed Q16 dip. This is consistent with the currently most favoured cometary breakup hypothesis, but nevertheless implies the complete breakup of 30 Comet 1/P Halley type objects. Finally, in the wide SCUBA-2 field-of-view we identify another candidate debris disc system that is potentially the largest yet discovered.
6 pages, 4 figures. Some figure resolutions reduced for file size limits. Submitted to MNRAS 11th December 2015
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- SCUBA-2: iterative map-making with the Sub-Millimetre User Reduction Facility
- Molecular Gas Clumps from the Destruction of Icy Bodies in the Pictoris Debris Disk
- FellWalker - a Clump Identification Algorithm
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- KIC 8462852: Transit of a Large Comet Family
- Tidal disruption of planetary bodies by white dwarfs II: Debris disc structure and ejected interstellar asteroids
- Families of Plausible Solutions to the Puzzle of Boyajian's Star
- The First Post-Kepler Brightness Dips of KIC 8462852
- KIC 8462852 Faded at an Average Rate of 0.165+-0.013 Magnitudes Per Century From 1890 To 1989
- KIC 8462852 Faded Throughout the Kepler Mission
- Modelling the KIC8462852 light curves: compatibility of the dips and secular dimming with an exocomet interpretation
- Secular Dimming of KIC 8462852 Following its Consumption of a Planet
- Mysterious eclipses in the light-curve of KIC8462852: a possible explanation
- Extinction and the Dimming of KIC 8462852
- Photometric and astrometric vagaries of the enigma star KIC 8462852
- Detection of a repeated transit signature in the light curve of the enigma star KIC 8462852: a 928-day period?
- Where Is the Flux Going? The Long-Term Photometric Variability of Boyajian's Star
- Sonneberg plate photometry for Boyajian's Star in two passbands
- The GALEX View of "Boyajian's Star" (KIC 8462852)
- Boyajian's Star B: The co-moving stellar companion to KIC 8462852
- The High Rate of the Boyajian's Star Anomaly as a Phenomenon
- Non-gray, Month-long Brightening of KIC 8462852 in the Immediate Aftermath of a Deep Dip
- High-resolution spectroscopy of Boyajian's star during optical dimming events
- Optical Polarimetry of KIC 8462852 in May-August 2017
- Extrasolar enigmas: from disintegrating exoplanets to exoasteroids