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The Outer Disks of Early-type Galaxies. II. Surface-brightness Profiles of Unbarred Galaxies and Trends with Hubble Type |
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A Strong Dichotomy in S0 Disk Profiles between the Virgo Cluster and the Field |
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Multi-layer Study of Wave Propagation in Sunspots |
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The Chromospheric Telescope |
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NIR spectral trends of HED meteorites: Can we discriminate between the magmatic evolution, mechanical mixing and observation geometry effects? |
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Variation in sunspot properties between 1999 and 2011 as observed with the Tenerife Infrared Polarimeter |
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Internal dynamics of Abell 2254: a merging galaxy cluster with a clumpy, diffuse radio emission |
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Orbit determination of close binary systems using lucky imaging |
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Environmental effects on the bright end of the galaxy luminosity function in galaxy clusters |
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The HST/ACS Coma Cluster Survey. IV. Intergalactic Globular Clusters and the Massive Globular Cluster System at the Core of the Coma Galaxy Cluster |
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The HST/ACS Coma Cluster Survey - III. Structural parameters of galaxies using single Sérsic fits |
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The HST/ACS Coma Cluster Survey - VI. Colour gradients in giant and dwarf early-type galaxies |
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The HST/ACS Coma Cluster Survey. VIII. Barred Disk Galaxies in the Core of the Coma Cluster |
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Detecting photons with orbital angular momentum in extended astronomical objects: application to solar observations |
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Testing the Unification Model for Active Galactic Nuclei in the Infrared: Are the Obscuring Tori of Type 1 and 2 Seyferts Different? |
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Torus and Active Galactic Nucleus Properties of Nearby Seyfert Galaxies: Results from Fitting Infrared Spectral Energy Distributions and Spectroscopy |
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Analytical maximum likelihood estimation of stellar magnetic fields |
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Seismology of Transversely Oscillating Coronal Loops with Siphon Flows |
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Damping Mechanisms for Oscillations in Solar Prominences |
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Bayesian Magnetohydrodynamic Seismology of Coronal Loops |
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Prominence Oscillations |
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Surface Alfvén Waves in Solar Flux Tubes |
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The Milky Way Tomography with SDSS. III. Stellar Kinematics |
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The Discovery of Binary White Dwarfs that will Merge Within 500 Myr |
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The ELM Survey. I. A Complete Sample of Extremely Low-mass White Dwarfs |
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