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Alpha element abundances and gradients in the Milky Way bulge from FLAMES-GIRAFFE spectra of 650 K giants |
iacweb |
6 months ago |
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Hubble Space Telescope and Ground-based Observations of V455 Andromedae Post-outburst |
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Discovery of the Near-infrared Counterpart to the Luminous Neutron-star Low-mass X-Ray Binary GX 3+1 |
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Plaskett's star: analysis of the CoRoT photometric data |
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A new gravitational wave verification source |
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The First Billion Years project: dark matter haloes going from contraction to expansion and back again |
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The structure of Abell 1351: a bimodal galaxy cluster with peculiar diffuse radio emission |
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UV surface brightness of galaxies from the local universe to z ~ 5 |
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Extinction Maps toward the Milky Way Bulge: Two-dimensional and Three-dimensional Tests with APOGEE |
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Fossil group origins. IV. Characterization of the sample and observational properties of fossil systems |
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Beam asymmetry Σ measurements of π- photoproduction on neutrons |
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Searching for solar siblings among the HARPS data |
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Properties of oscillatory motions in a facular region |
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Serendipitous detection of an overdensity of Herschel-SPIRE 250 μm sources south of MRC 1138-26 |
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Bottom-heavy initial mass function in a nearby compact L★ galaxy |
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GRB 081007 and GRB 090424: The Surrounding Medium, Outflows, and Supernovae |
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X-ray emission from RX J1720.1+2638 and Abell 267: A comparison between a fossil and a non-fossil system |
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The 2011 Periastron Passage of the Be Binary δ Scorpii |
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First results of an Hα based search of classical Be stars in the Perseus Arm and beyond |
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Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal |
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The optical counterpart of the bright X-ray transient Swift J1745-26 |
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LOFT: the Large Observatory For X-ray Timing |
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Properties of convective motions in facular regions |
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Automated Unsupervised Classification of the Sloan Digital Sky Survey Stellar Spectra using k-means Clustering |
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Turbulent eddy-time-correlation in the solar convective zone |
iacweb |
6 months ago |
