S stars without technetium - The binary star connection

S stars: infrared colors, technetium, and binarity

S sub q and L sub q variations at Kakioka, Memambetsu and Kanoya, Japan, 1958-1973

S times from deep-focus Indian earthquakes

S to P Conversion as an Aid to Crustal Studies

S to P scattering at the 650 km discontinuity

S to P wave form factors in semi-leptonic B decays

S U Cassiopei&aelig

S V effective collision strengths (Hudson+, 2006)

S V line ratios in the sun

S V Persei.

S velocities in D" from diffracted SH-waves at the core boundary

S velocity reversal in the mantle transition zone

S velocity structure and radial anisotropy in the Aegean region from surface wave dispersion

S VI line ratios in the sun

S Vulpeculae

S Vulpeculae.

S wave attenuation in the coastal region of Jalisco-Colima, México

S wave Kπscattering and effects of κin J/ψ\to {\bar K}^{*0}(892)K^+π^-

S wave meson spectra from the light cone harmonic oscillator model with a consistent hyperfine interaction