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The evolution and delivery of rocky extra-solar materials to white dwarfs
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Understanding stellar evolution and its effect on planetary systems is crucial for correctly interpreting the chemical constraints of exo-planetary material that can be given to us by white dwarfs. This article will describe how asteroids, moons, and comets, as well as boulders, pebbles and dust, evolve into eventual targets for chemical spectroscopy, and how planets and companion stars play a vital role in reshaping system architectures for this purpose.
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Cited by 2 Pith papers
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A Search for Transiting Exocomets in TESS Sectors 1-26
A TESS primary mission search finds five new exocomet-like transit candidates and estimates a 2.64e-4 per star per year occurrence rate, concluding such transits are rare at 0.1% to 1% depths.
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Chemical evolution of an evaporating lava pool
An evaporating lava pool reaches a steady state where the escaping atmosphere has the same composition as mantle material melted into the pool, so dust tails of disintegrating planets can trace interior composition.
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