Post-Main-Sequence Evolution of Icy Minor Planets. III. Water Retention in Dwarf Planets and Exomoons and Implications for White Dwarf Pollution
Uri Malamud and Hagai B. Perets 2017 ApJ 849 8
Icy minor planets are shown to typically retain some of their water through their host star’s evolution into a white dwarf, allowing them to potentially pollute the white dwarf’s atmosphere after a later collision.