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Star Formation Rate Estimators: [OII]3727 vs Hα for Local Star-forming Galaxies |
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1 year 5 months ago |
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Low Metallicity Stars in SDSS and SEGUE |
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Ground-based observations of the β Cephei CoRoT main target HD 180 642: abundance analysis and mode identification |
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Hot Horizontal Branch Stars in ω Centauri: Clues about their Origin from the Cluster Color Magnitude Diagram |
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1 year 5 months ago |
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The First Precise Determination of an Optical-Far-Ultraviolet Extinction Curve Beyond the Local Group (z=0.83) |
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1 year 5 months ago |
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Non-circular motion evidence in the circumnuclear region of M100 (NGC 4321) |
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1 year 5 months ago |
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Discovery of a galactic wind in the central region of M100 |
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1 year 5 months ago |
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Determination of field strengths in the quiet Sun |
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Scattering polarization of hydrogen lines in the presence of turbulent electric fields |
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A near-infrared survey for new low-mass members in α Per |
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Discovery of Kilohertz Quasi-periodic Oscillations and Shifted Frequency Correlations in the Accreting Millisecond Pulsar XTE J1807-294 |
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Abundances of Na, Mg and Al in stars with giant planets |
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Oxygen abundances in planet-harbouring stars. Comparison of different abundance indicators |
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The Proper Motion of the Magellanic Clouds. I. First Results and Description of the Program |
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A photometric redshift of z = 1.8{+0.4}{-0.3} for the AGILE GRB 080514B |
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MAGIC Observations of the Unidentified γ-Ray Source TeV J2032+4130 |
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Optical and infrared photometry of new very low-mass stars and brown dwarfs in the sigma Orionis cluster |
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Relation between photospheric magnetic field and chromospheric emission |
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Near-IR internetwork spectro-polarimetry at different heliocentric angles |
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Intracluster Stellar Population Properties from N-Body Cosmological Simulations. I. Constraints at z = 0 |
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Multiepoch Multiwavelength Spectra and Models for Blazar 3C 279 |
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Galactic evolution of the light-element isotopes |
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The 1991 outburst of Comet P/Metcalf-Brewington: A study of the light curve |
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Net Circular Polarization in Magnetic Spectral Lines Produced by Velocity Gradients: Some Analytical Results |
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Infrared flux excesses from hot subdwarfs. II. 72 more objects |
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1 year 5 months ago |
