| Publication |
On the importance of the few most massive stars: The ionizing cluster of NGC 588 |
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10 months 1 week ago |
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Kinematic Modelling of the Sculptor Dwarf Spheroidal Galaxy |
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10 months 1 week ago |
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The Metallicity of Pregalactic Globular Clusters: The Observational Consequences of the First Stars |
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10 months 1 week ago |
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Kinematics of globular cluster systems and the formation of early-type galaxies |
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10 months 1 week ago |
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Performance of satellite-to-ground communications link between ARTEMIS and the Optical Ground Station |
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Observation of enhanced X-ray emission from the CTTS AA Tauri during one transit of an accretion funnel flow |
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Helioseismology program for the PICARD satellite |
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The Fundamental Plane for early-type galaxies: dependence on the magnitude range |
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Discovery of Two Very Low Mass Binaries: Final Results of an Adaptive Optics Survey of Nearby M6.0-M7.5 Stars |
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B-type supergiants in the Small Magellanic Cloud: rotational velocities and implications for evolutionary models |
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Lines in the cosmic microwave background spectrum from the epoch of cosmological hydrogen recombination |
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Upper limits on gravitational wave bursts in LIGO's second science run |
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Status of the GEO600 detector |
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The High-Excitation Planetary Nebula NGC 246: Optical and Near-Ultraviolet Observations and Two-dimensional Numerical Models |
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The Araucaria Project: A Wide-Field Photometric Survey for Cepheid Variables in NGC 3109 |
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The Remarkable Alternating Spectra of the Of?p Star HD 191612 |
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Search for photospheric footpoints of quiet Sun transition region loops |
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Fast MHD oscillations of a 3-dimensional prominence fibril |
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Slow MHD oscillations in density structured coronal loops |
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The Ca II Infrared Triplet Lines as Diagnostics of Chromospheric Magnetism |
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Using symmetries and generating functions to calculate and minimize moments of inertia |
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B -> X_s gamma and B^+ -> l^+
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Wide Range Neutron Flux Measuring Channel for Aerospace Application |
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Ultraluminous X-ray Sources: Bubbles and Optical Counterparts |
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Dark bursts in the Swift era |
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