Tipo de publicación: Con árbitro

  • Publicación
    A Comparison Between Near-Infrared And Visible Imaging Of The Inner Coma Of Comet Hale-Bopp At Perihelion
    We present a comparison between images of comet C/1995 O1 (Hale-Bopp) obtained from 12 March to 9 May 1997, with two telescopes of the Observatorio del Teide...
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    A comparison between the soft X-ray and [O III] morphologies of active galactic nuclei
    Several studies of nearby active galactic nuclei (AGNs) have shown that the soft X-ray emission presents a size and morphology resembling that of the narrow...
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    A comparison between X-shooter spectra and PHOENIX models across the HR-diagram
    Aims: The path towards robust near-infrared extensions of stellar population models involves the confrontation between empirical and synthetic stellar spectral...
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    A comparison of galaxy group luminosity functions from semi-analytic models
    Semi-analytic models (SAMs) are currently one of the primary tools with which we model statistically significant ensembles of galaxies. The underlying physical...
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    A Complete Multiwavelength Characterization of Faint Chandra X-Ray Sources Seen in the Spitzer Wide-Area Infrared Extragalactic (SWIRE) Survey
    We exploit deep combined observations with Spitzer and Chandra of the Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE) in the ELAIS N1 region to...
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    A complex bipolar outflow in the Wolf-Rayet BCDG He 2-10
    We present results from multi-wavelength observations of the Wolf-Rayet (WR) blue compact dwarf galaxy He 2-10. These observations include Hα and optical red...
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    A complex state transition from the black hole candidate Swift J1753.5-0127
    We present our monitoring campaign of the outburst of the black hole candidate Swift J1753.5-0127, observed with the Rossi X-ray Timing Explorer and the Swift...
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    A composite H ii region luminosity function in Hα of unprecedented statistical weight
    Context: .Statistical properties of H ii region populations in disk galaxies yield important clues to the physics of massive star formation. Aims: .We present a...
  • Publicación
    A compositional link between rocky exoplanets and their host stars
    Stars and planets both form by accreting material from a surrounding disk. Because they grow from the same material, theory predicts that there should be a...