Why Galaxies Care about Post-AGB stars
Why isn't the solar constant a constant?
Why one-dimensional models fail in the diagnosis of average spectra from inhomogeneous stellar atmospheres
Why the sunspot cycle is double peaked
Why variable AGB stars with Long Secondary Periods aren't binaries, but are dusty
Wide Binary Stars in the Galactic Field - A Statistical Approach
Wide double stars - I. The spectroscopic binaries: Double stars with wide separations in the AGK3 - I. The components that are themselves spectroscopic binaries
Wide Field Wavefront Sensing
Wide-field Infrared Survey Explorer Observations of Young Stellar Objects in the Western Circinus Molecular Cloud
Wide-Field Survey of Emission-line Stars in IC 1396
Widespread nanoflare variability detected with Hinode/XRT in a solar active region
Width of Sunspot Generating Zone and Reconstruction of Butterfly Diagram
Wind modelling of very massive stars up to 300 solar masses
Wind Models for Very Massive Stars in the Local Universe
Wind structure and luminosity variations in the WR/LBV HD 5980
Wind structure in late-B supergiants
Wind-accretion disks in wide binaries, second generation protoplanetary disks and accretion onto white dwarfs
Wind-driving protostellar accretion discs. I. Formulation and parameter constraints
Wind-driving protostellar accretion discs. II. Numerical method and illustrative solutions
Winds from Luminous Late-Type Stars: II. Broadband Frequency Distribution of Alfvén Waves