The Photoevaporative Wind from the Disk of TW Hya
The physical properties of extrasolar planets
The Physics of Protoplanetesimal Dust Agglomerates. III. Compaction in Multiple Collisions
The Physics of Protoplanetesimal Dust Agglomerates. IV. Towards a Dynamical Collision Model
The Physics of Protoplanetesimal Dust Agglomerates. V. Multiple Impacts of Dusty Agglomerates at Velocities Above the Fragmentation Threshold
The Physics of Protoplanetesimal Dust Agglomerates. Vi. Erosion of Large Aggregates as a Source of Micrometer-Sized Particles
The physics of wind-blown sand and dust
The Planets around the Post-Common Envelope Binary NN Serpentis
The population of natural Earth satellites
The Posterior Distribution of sin(i) for Exoplanets with M_T sin(i) Determined from Radial Velocity Data
The Posterior Distribution of sin(i) Values For Exoplanets With M_T sin(i) Determined From Radial Velocity Data
The Potato Radius: a Lower Minimum Size for Dwarf Planets
The Potential Importance of Non-Local, Deep Transport on the Energetics, Momentum, Chemistry, and Aerosol Distributions in the Atmospheres of Earth, Mars and Titan
The Potential of the Timing Method to Detect Evolved Planetary Systems
The propeller and the frog
The properties of asteroid (2867) Steins from Spitzer observations and OSIRIS shape reconstruction
The Properties of Prestellar Discs in Isolated and Multiple Prestellar Systems
The Pulsar Planets: A Test Case of Terrestrial Planet Assembly
The Radial Velocity TATOOINE Search for Circumbinary Planets: Planet Detection Limits for a Sample of Double-lined Binary Stars - Initial Results from Keck I/Hires, Shane/CAT/Hamspec and TNG/Sarg Observations
The rate of thermal atmospheric escape