WD 1145+017 Photometric Observations During 8 Months of High Activity
B.L. Gary, S. Rappaport, T.G. Kaye, R. Alonso, F.-J. Hambsch

TL;DR
This study presents eight months of photometric observations of WD 1145+017, revealing dynamic dust cloud activity, multiple transient events, and insights into dust production mechanisms around the white dwarf.
Contribution
It provides detailed observational data on dust cloud behavior and evolution, highlighting the need for multiple dust production mechanisms around WD 1145+017.
Findings
Multiple dust cloud events with distinct periods observed.
Dust activity varied significantly over the observation period.
Collisions and other mechanisms contribute to dust production.
Abstract
WD 1145+017 was observed from 2015 November to 2016 July for the purpose of characterizing transit behavior of the white dwarf by dust clouds thought to be produced by fragments of an asteroid in close orbit with the star. Fortuitously, most of these observations were carried out during a time when the overall `dip' activity was dramatically enhanced over that during its discovery with Kepler K2. By the end of our reported observations the dip activity had declined to a level close to its K2 discovery state. Three notable events were observed. In 2016 January a large number of dust clouds appeared that had an orbital period of 4.4912 hours, and this event also marked the end of a 3-month interval dominated by the K2 `A' period. The second event was a 2016 April 21 appearance of four dip features with drift lines in a waterfall diagram (date vs. phase) that diverged from their origin…
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