Are the magnetic fields of millisecond pulsars ~ 10^8 G?

Are the outflows in FU Orionis systems driven by the stellar magnetic field?

Are the photospheric sunspots magnetically force-free in nature?

Are the spin axes of stars randomly aligned within a cluster?

Are the Stellar Winds in IC1613 stronger than expected?

Are There Age Spreads in Star Forming Regions?

Are there any stable magnetic fields in barotropic stars?

Arrival time calculation for interplanetary coronal mass ejections with circular fronts and application to STEREO observations of the 2009 February 13 eruption

ARTEMIS IV Radio Observations of the 14 July 2000 Large Solar Event

ASAS Light Curves of Intermediate Mass Eclipsing Binaries and the Parameters of HI Mon

ASAS photometry of ROSAT sources I. Periodic variable stars coincident with bright sources from ROSAT all sky survey

Aspects of Multi-Dimensional Modelling of Substellar Atmospheres

Aspects of observational red giant population seismology

Assessing the accuracy of the gravity determination in late-type stars with solar-like pulsators

Assessing the Role of Spin Noise in the Precision Timing of Millisecond Pulsars

Assimilating data into an αω dynamo model of the sun: A variational approach

Asteroseismic analysis of the CoRoT δ-Scuti star HD174936

Asteroseismic analysis of the roAp star alpha Circini: 84 days of high-precision photometry from the WIRE satellite

Asteroseismic constraints on diffusion in WD envelopes

Asteroseismic determination of the physical characteristics of the planetary system host HR\,8799 ($λ$ Bootis nature and age)