The Solar Neighborhood. XXVI. AP Col: The Closest (8.4 pc) Pre-Main-Sequence Star
The Solar Orbiter mission and its prospects for helioseismology
The solar photospheric abundance of carbon.Analysis of atomic carbon lines with the CO5BOLD solar model
The solar photospheric abundance of zirconium
The solar photospheric nitrogen abundance. Analysis of atomic transitions with 3D and 1D model atmospheres
The Solar Photospheric Nitrogen Abundance: Determination with 3D and 1D Model Atmospheres
The Solar Photospheric-to-Coronal Fe abundance from X-ray Fluorescence Lines
The Solar Spectroscopy Explorer Mission
The solar type protostar IRAS16293-2422: new constraints on the physical structure
The solar wind as seen by SOHO/SWAN since 1996: comparison with SOHO/LASCO C2 coronal densities
The Solar Wind Energy Flux
The solar X-ray continuum measured by RESIK
The solar, exoplanet and cosmological lithium problems
The solar-like CoRoT target HD 170987: spectroscopic and seismic observations
The Solar-Type Contact Binary BX Pegasi Revisited
The space density and X-ray luminosity function of non-magnetic cataclysmic variables
The Space Interferometry Mission Astrometric Grid Giant-Star Survey. III. Basic Stellar Parameters for an Extended Sample
The spatial damping of magnetohydrodynamic waves in a flowing partially ionised prominence plasma
The Spatial Distribution of Star Formation in the Solar Neighbourhood: Do all stars form in clusters?
The spatial distribution of stars in open clusters