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A photometric study of globular clusters observed by the APOGEE survey |
iacweb |
Hace 1 year 10 months |
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Membership, lithium and chromospheric activity of the young open clusters IC 2391, IC 2602 and IC 4665 from GES (Gaia-ESO Survey) observations |
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Hace 1 year 10 months |
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Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud |
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Hace 1 year 10 months |
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The Absolute Age of the Globular Cluster M15 Using Near-infrared Adaptive Optics Images from PISCES/LBT. |
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Hace 1 year 10 months |
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Beyond MHD: modeling and observation of partially ionized solar plasma processes |
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Mass accretion rates from multiband photometry in the Carina Nebula: the case of Trumpler 14 |
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Probing the z > 6 Universe with the First Hubble Frontier Fields Cluster A2744 |
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The deep spectrophotometric mosaic of the Orion Nebula. Preliminary results |
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On the Density Profile of the Globular Cluster M92 |
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Fully cosmological virtual massive galaxies at z = 0: kinematical, morphological and stellar population characterization |
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Cosmological constraints on nonstandard inflationary quantum collapse models |
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Star formation history of KDG61 and KDG64 from spectroscopy and colour-magnitude diagrams |
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The Sun, the Solar Wind, and the Heliosphere |
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A pilot study for the SCUBA-2 `All-Sky' Survey |
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Small-spatial-scale variations of nebular properties and the abundance discrepancy in three Galactic HII regions |
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CCD Photometry of M15 |
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BeX systems as seen by INTEGRAL |
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Further evidence for the presence of a neutron star in 4U 2206+54. INTEGRAL and VLA observations |
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Stars at Low Metallicity in Dwarf Galaxies |
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Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121 |
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High-Precision Near-Infrared Photometry of a Large Sample of Bright Stars Visible from the Northern Hemisphere |
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Strategies for Imaging Faint Extended Sources in the Near-Infrared |
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On the ultracompact nature of 4U1822-000 |
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DQ white-dwarf stars with low C abundance: possible progenitors |
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On the Relative Distances of ω Centauri and 47 Tucanae |
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Hace 1 year 10 months |
