Explaining the variability of WD 1145+017 with simulations of asteroid tidal disruption
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DOI: 10.1093/mnras/stw2748
Abstract: Post-main-sequence planetary science has been galvanised by the striking variability, depth and shape of the photometric transit curves due to objects orbiting white dwarf WD 1145+017, a star which also hosts a dusty debris disc… read more here.
Keywords: 1145 017; 017 simulations; disruption; variability 1145 ... See more keywords