Confirmation of simultaneous p and g mode excitation in HD 8801 and Gamma Peg from time-resolved multicolour photometry of six candidate "hybrid" pulsators

Confirmation of the magnetic oblique rotator model for the Of?p star HD 191612

Confirmation of the occurrence of the Hall instability in the non-linear regime

Confirmation of the VeLLO L1148-IRS: Star Formation at very low (Column) Density

Confirming Fundamental Parameters of the Exoplanet Host Star epsilon Eridani Using the Navy Optical Interferometer

Confirming the Primarily Smooth Structure of the Vega Debris Disk at Millimeter Wavelengths

Confronting 3 Dimensional Time-dependent Jet Simulations with HST Observations

Confronting Substellar Theoretical Models with Stellar Ages

Conical Winds from the Disk-Magnetosphere Boundary

Connecting planets around horizontal branch stars with known exoplanets

Connecting Recurrent Novae to [some] Type Ia Supernovae

Connecting RS OPh to [some] Type Ia Supernovae

Connecting the Sun and the Solar Wind: The First 2.5 Dimensional Self-consistent MHD Simulation under the Alfvén Wave Scenario

Connections Between Tilted Accretion Disks Around White Dwarfs and Substellar Companions

Consequences of Magnetic Field Structure for Heat Transport in Magnetohydrodynamics

Constants of motion in stationary axisymmetric gravitational fields

Constrained fitting of disentangled binary spectra: application to V615 Per in the open cluster h Persei

Constraining 3D Magnetic Field Extrapolations Using The Twin Perspectives of STEREO

Constraining Ceres' interior from its Rotational Motion

Constraining Low-Frequency Alfvenic Turbulence in the Solar Wind Using Density Fluctuation Measurements