1. Thermal convection in an initially compositionally stratified fluid heated from below: Application to a model for the evolution of the Moon;Alley,1996
2. Estimates of cryptomare thickness and volume in Schiller–Schickard, Mare Humorum and Oceanus Procellarum areas;Antonenko,1995
3. The nature of isostasy on the Moon;Baldwin;Phys. Earth Planet. Int.,1971
4. The tsunami model of the origin of ring structures concentric with large lunar craters;Baldwin;Phys. Earth Planet. Int.,1972
5. The deep structure of lunar basins: Implications for basin formation and modification;Bratt;J. Geophys. Res.,1985