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A new analysis of the 11-year period in OJ287 - Confirmation of its existence |
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On the massive star-forming capacity of molecular clouds |
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Constraints on cosmological parameters from recent measurements of cosmic microwave background anisotropy |
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Library of high-resolution UES echelle spectra of F, G, K and M field dwarf stars |
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Stellar evolution models for Z = 0.0001 to 0.03 |
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Atlas of H alpha Emission of a Sample of Nearby Hickson Compact Groups of Galaxies |
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Adaptation of streetlighting on La Palma |
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Photometric variability of LBV-candidate stars and Hubble-Sandage variables A, B, C and 2 in M 33 |
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EROS 2 proper motion survey: a field brown dwarf, and an L dwarf companion to LHS 102 |
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On the parallax of WD 0346++246: a halo white dwarf candidate |
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1st Advances in Solar Physics Euroconference: Advances in the Physics of Sunspots |
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PN G135.9+55.9: a New, Extremely Oxygen-Poor Planetary Nebula in the Galactic Halo |
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Supernovae 1992R and 1992ac in MCG +10-24-007 |
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Gas and Dust Emission from the Nuclear Region of the Circinus Galaxy |
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The Nature of the Nuclear H2O Masers of NGC 1068: Reverberation and Evidence for a Rotating Disk Geometry |
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Taiwan Oscillation Network |
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The grey behaviour of Saharan dust |
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The wind momentum-luminosity relationship of galactic A- and B-supergiants |
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Fundamental parameters of Galactic luminous OB stars VI. Temperatures, masses and WLR of Cyg OB2 supergiants |
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The age-mass relation for chromospherically active binaries. III. Lithium depletion in giant components |
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Chromospheric polarity reversals on sunspots. Are they consistent with weak line emission? |
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Physical Properties of the Solar Magnetic Photosphere under the MISMA Hypothesis. I. Description of the Inversion Procedure |
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The photosphere and chromosphere of the RS Canum Venaticorum star, II Pegasi. II. A multi-wavelength campaign in August/September 1992 |
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Infrared light curves and absolute stellar parameters of the Algol system δ Librae: is δ Librae really an overmassive Algol binary? |
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The interacting system NGC 7753-7752 (Arp 86). I - BVRI photometry |
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