Non-grey dimming events of KIC 8462852 from GTC spectrophotometry
arXiv:1801.00720 · doi:10.1051/0004-6361/201732453
Abstract
We report ground-based spectrophotometry of KIC 8462852, during its first dimming events since the end of the Kepler mission. The dimmings show a clear colour-signature, and are deeper in visual blue wavelengths than in red ones. The flux loss' wavelength dependency can be described with an Ångström absorption coefficient of , which is compatible with absorption by optically thin dust with particle sizes on the order of 0.0015 to 0.15 m. These particles would be smaller than is required to be resistant against blow-out by radiation pressure when close to the star. During occultation events, these particles must be replenished on time-scales of days. If dust is indeed the source of KIC 8462852's dimming events, deeper dimming events should show more neutral colours, as is expected from optically thick absorbers.
5 pages, accepted for A&A letters
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- A Large Ground-Based Observing Campaign of the Disintegrating Planet K2-22b
- The KIC 8462852 Light Curve From 2015.75 to 2018.18 Shows a Variable Secular Decline
- Sudden extreme obscuration of a Sun-like main-sequence star: evolution of the circumstellar dust around ASASSN-21qj
- 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
- Extrasolar enigmas: from disintegrating exoplanets to exoasteroids