Tidal breakup of cohesive rubble piles around white dwarfs imposes a 0.1-1 km maximum fragment size that sets the initial debris distribution and requires collisional grinding before Poynting-Robertson drag acts.
T., Kilic, M., Lisse, C
2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
The paper advocates preserving HST UV spectroscopy through 2035 as essential for statistically significant samples of polluted white dwarf compositions, groundwork for HWO, and synergy with JWST.
citing papers explorer
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Size limits on tidal debris around white dwarfs: the km-size barrier
Tidal breakup of cohesive rubble piles around white dwarfs imposes a 0.1-1 km maximum fragment size that sets the initial debris distribution and requires collisional grinding before Poynting-Robertson drag acts.
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From Hubble to HWO: Bridging the Frontier of White Dwarf Exoplanet Science
The paper advocates preserving HST UV spectroscopy through 2035 as essential for statistically significant samples of polluted white dwarf compositions, groundwork for HWO, and synergy with JWST.