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The 3-D topology of magnetic fields in and around sunspots |
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The Nature of Luminous X-Ray Sources with Mid-Infrared Counterparts |
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Globular cluster systems of six shell galaxies |
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Warm Water Vapor around Sagittarius B2 |
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Multiline Zeeman signatures through line addition |
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The bright galaxy population of five medium redshift clusters. I. Color-magnitude relation, blue fractions, and visual morphology |
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Near-Infrared Galaxy Counts and Evolution from the Wide-Field ALHAMBRA Survey |
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The bright galaxy population of five medium redshift clusters. II. Quantitative galaxy morphology |
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Infrared mergers and infrared quasi-stellar objects with galactic winds - II. NGC5514: two extranuclear starbursts with LINER properties and a supergiant bubble in the rupture phase |
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Unveiling the Narrow-Line Seyfert 1 Nature of Markarian 573 Using Near-Infrared Spectroscopy |
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Gamma-ray line emission from OB associations and young open clusters. II. The Cygnus region |
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The Mass Function at the End of the Main Sequence: The M35 Open Cluster |
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Radio to γ-ray observations of 3C 454.3:1993-1995 |
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A Morphological Type Dependence in the μ0-log h Plane of Spiral Galaxy Disks |
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Library of high-resolution UES echelle spectra of F, G, K and M field dwarf stars |
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The age-mass relation for chromospherically active binaries. II. Lithium depletion in dwarf components. |
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Spectrophotometric Observations of Blue Compact Dwarf Galaxies: Mkn 36 and Mkn 370 |
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HII region luminosity functions: A new standard candle for extragalactic distances? |
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HII Region Luminosity Functions: Derivation of a New Standard Candle for Extragalactic Distances |
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Aquila X-1: a low-inclination soft X-ray transient |
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Optical surface photometry of radio galaxies. II. Observations and data analysis |
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Quantitative spectroscopic criteria for the classification of pre-main sequence low-mass stars. |
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A Far-Infrared Study of the CfA Seyfert Sample. I. The Data |
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Evidence for Diverse Optical Emission from Gamma-Ray Burst Sources |
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Thermal properties of magnetic flux tubes. I. Solution of the diffusion problem |
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