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The circumnuclear region in the Seyfert 1 galaxy NGC 3227 |
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Phase differences between luminosity and velocity measurements of the acoustic modes |
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Evolutionary versus dynamical time scales for the evolution of the central stars of planetary nebulae |
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Galactic evolution of beryllium. I. NLTE effects and accuracy of beryllium abundances in metal-poor stars. |
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Spectral signature of uncombed penumbral magnetic fields. Comment |
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Thermal Relaxation of Very Small Solar Magnetic Structures in Intergranules: A Process That Produces Kilogauss Magnetic Field Strengths |
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On the optical variability of the QSO PKS 2128-123 |
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An X-ray survey of extragalactic radio jets with Chandra |
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Analysis of low frequency signal with the GOLF experiment: methodology and results |
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Complex poles and oscillatory screened potential in QED plasmas |
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Linewidth of low degree acoustic modes of the Sun |
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g-mode: a new generation of helioseismic instrument |
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The magnetic field in the convection zone as a link between the active regions on the surface and the field in the solar interior |
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LIRIS: a long-slit intermediate-resolution infrared spectrograph for the WHT |
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The bipolar H II region S 201 |
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GRB 011121. |
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Obituary: Victor Amazaspovich Ambartsumian, 1912 [i.e. 1908] -1996 |
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ISOPHOT: far-infrared imaging, polarimetry, and spectrophotometry on ISO |
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Is the Milky Way a Double-barred Galaxy? |
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GRO J0422+32 |
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Detectability of Jupiter-to-Brown-Dwarf-Mass Companions Around Small Eclipsing Binary Systems |
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J1859+226 |
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Solar Polarization |
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Towards a Reliable Diagnostics of `Turbulent' Magnetic Fields Via the Hanle Effect in the Sr I λ4607 Å Line |
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STEPHI-92 - Bn-Cancri and Bu-Cancri - Two Delta-Scuties in the Praesepe Cluster |
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