planets and satellites: individual: KIC 12557548b

Dusty tails of evaporating exoplanets. II. Physical modelling of the KIC 12557548b light curve

Context. Evaporating rocky exoplanets, such as KIC 12557548b, eject large amounts of dust, which can trail the planet in a comet- like tail. When such objects occult their host star, the resulting transit signal contains information about the dust in …