| Publicación |
Temporal Evolution of the Scattering Polarization of the Ca II IR Triplet in Hydrodynamical Models of the Solar Chromosphere |
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Microlensing of Quasar Broad Emission Lines: Constraints on Broad Line Region Size |
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Systematic variation of the stellar initial mass function with velocity dispersion in early-type galaxies |
iacweb |
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The Chandra X-Ray Survey of Planetary Nebulae (CHANPLANS): Probing Binarity, Magnetic Fields, and Wind Collisions |
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LOFT: the Large Observatory For X-ray Timing |
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Chromospheric Lyman-alpha spectro-polarimeter (CLASP) |
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No surviving evolved companions of the progenitor of SN1006 |
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The hypergiant HR 8752 evolving through the yellow evolutionary void |
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Intermediate Resolution Near-infrared Spectroscopy of 36 Late M Dwarfs |
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Power Spectra of Velocities and Magnetic Fields on the Solar Surface and their Dependence on the Unsigned Magnetic Flux Density |
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LEMUR: Large European module for solar Ultraviolet Research. European contribution to JAXA's Solar-C mission |
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The optical SN 2012bz associated with the long GRB 120422A |
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Spectral Energy Distributions of Type 1 Active Galactic Nuclei in the COSMOS Survey. I. The XMM-COSMOS Sample |
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Breaks in Thin and Thick Disks of Edge-on Galaxies Imaged in the Spitzer Survey Stellar Structure in Galaxies (S4G) |
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Astrometric and photometric initial mass functions from the UKIDSS Galactic Clusters Survey - II. The Alpha Persei open cluster |
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Excitation of emission lines by fluorescence and recombination in IC 418 |
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Astrometric and photometric initial mass functions from the UKIDSS Galactic Clusters Survey - III. Praesepe |
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The influence of bars in the star formation history and chemical evolution of disk galaxies |
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A multi-wavelength analysis of M 81: insight on the nature of Arp's loop |
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Herschel-ATLAS: The dust energy balance in the edge-on spiral galaxy UGC 4754 |
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A Seismic Signature of a Second Dynamo? |
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K 3-22: a D-type symbiotic star |
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The Peculiar Optical Spectrum of 4C+22.25: Imprint of a Massive Black Hole Binary? |
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Shear Photospheric Forcing and the Origin of Turbulence in Coronal Loops |
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Was the progenitor of the Sagittarius stream a disc galaxy? |
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