Population Synthesis of Hot Subdwarfs: A Parameter Study
Positions and sizes of X-ray solar flare sources
Possible constraints on exoplanet magnetic field strengths from planet-star interaction
Possible detection of two giant extrasolar planets orbiting the eclipsing polar UZ Fornacis
Possible explanations of the Maunder minimum from a flux transport dynamo model
Possible Implications of the Planet Orbiting the Red Horizontal Branch Star HIP 13044
Possible optical counterpart of PSR J1357-6429
Possible planet-forming regions on submillimetre images
Possible Signatures of Magnetospheric Accretion onto Young Giant Planets
Post common envelope binaries from SDSS. IV: SDSSJ121258.25-012310.1, a new eclipsing system
Post common envelope binaries from SDSS. XII: The orbital period distribution
Post Common Envelope Binaries from SDSS. XV: Accurate stellar parameters for a cool 0.4-solar mass white dwarf and a 0.16-solar mass M-dwarf in a 3 hour eclipsing binary
Post common envelope binaries from the SDSS. VI. SDSS J120615.73+510047.0: a new low accretion rate magnetic binary
Post-AGB stars in the AKARI survey
Post-AGB stars in the SMC as tracers of stellar evolution: the extreme s-process enrichment of the 21 micrometer star J004441.04-732136.4
Post-AGB Stars with Circumbinary Discs
Post-AGB stars with hot circumstellar dust: binarity of the low-amplitude pulsators
Post-common envelope binaries from SDSS - VII: A catalogue of white dwarf-main sequence binaries
Post-common envelope binaries from SDSS - XIV. The DR7 white dwarf-main sequence binary catalogue
Post-common envelope binaries from SDSS - XVI. Long orbital period systems and the energy budget of CE evolution