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The Star Formation History and Morphological Evolution of the Draco Dwarf Spheroidal Galaxy |
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3 weeks 6 days ago |
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The Star Formation History and Spatial Distribution of Stellar Populations in the Ursa Minor Dwarf Spheroidal Galaxy |
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On the Shape of the Light Profiles of Early Type Galaxies |
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A survey of the ISM in early-type galaxies. I. The ionized gas. |
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Unveiling the Active Nucleus of Centaurus A |
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Multiband Analysis of a Sample of Blue Compact Dwarf Galaxies. I. Surface Brightness Distribution, Morphology, and Structural Parameters |
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On the estimation of galaxy structural parameters: the Sérsic model |
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Old stellar Galactic disc in near-plane regions according to 2MASS: Scales, cut-off, flare and warp |
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Iterative Methods for the Non-LTE Transfer of Polarized Radiation: Resonance Line Polarization in One-dimensional Atmospheres |
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Non-LTE Inversion of Stokes Profiles Induced by the Zeeman Effect |
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The Iron Line Formation Problem in Three-dimensional Hydrodynamic Models of Solar-like Photospheres |
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Selective absorption processes as the origin of puzzling spectral line polarization from the Sun |
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Time Series of Solar Granulation Images. II. Evolution of Individual Granules |
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Seismology of delta Scuti stars in the Praesepe cluster. II. Identification of radial modes and their associated stellar parameters |
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Seismology of delta Scuti stars in the Praesepe cluster. I. Ranges of unstable modes as predicted by linear analysis versus observations |
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delta Scuti stars in Praesepe I. The STACC 1998 campaign - the photometry |
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Discovery of Young, Isolated Planetary Mass Objects in the σ Orionis Star Cluster |
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An upper limit to the abundance of Be-9 in the Population II star HD 76932 from a high resolution spectrum with IUE |
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Lithium abundances in metal-deficient dwarfs |
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Star Formation Triggering by Density Waves in the Grand Design Spirals NGC 3992 and NGC 628 |
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The nature of arms in spiral galaxies. I - Azimuthal colour profiles of NGC 7479 and NGC 1832 |
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The Central Region in M100: Observations and Modeling |
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Molecular Cloudlets Embedded in a Diffuse H i Cloud within 120 Parsecs of the Sun |
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A New Chemo-evolutionary Population Synthesis Model for Early-Type Galaxies. I. Theoretical Basis |
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Global morphology and physical relations between the stars, gas and dust in the disc and arms of M100. |
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