Tipo de publicación: Sin árbitro

  • Publicación
    The influence of spot saturation on DIMM seeing measurements
    The DIMM is a widely accepted and often used instrument for seeing measurements. Nevertheless, its incorrect use may give rise to errors in seeing values. A...
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    The Influence of the Environment on Bar Formation
    Galaxy mergers and interactions are mechanisms which should drive the formation of bars. Therefore, we could expect that the fraction of barred galaxies...
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    The infrared counterpart of GX 17+2
    We present Keck K-band observations of GX 17+2 which reveal a bright counterpart in the radio error circle of Deutsch et al. (1999), coincident with their star...
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    The Infrared Nuclear Emission of Seyfert Galaxies on Parsec Scales: Testing the Clumpy Torus Models
    Not Available
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    The Infrared Nuclear Emission of Seyfert Galaxies on Parsec Scales: Testing the Clumpy Torus Models
    We present subarcsecond resolution mid-infrared (mid-IR) photometry in the range from 8 to 20 μm of 18 nearby Seyfert galaxies, reporting high spatial...
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    The infrared overluminosity of young, ultracool substellar objects
    Most young, ultracool substellar objects with spectral types later than M9 show very red mid-infrared colors up to 24~micron, significantly redder than expected...
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    The initial lithium abundance of T Tauri stars.
    Not Available
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    The Initial--Final Mass Relationship of White Dwarfs in Common Proper Motion Pairs
    A promising approach to decrease the uncertainties in the initial--final mass relationship, which is still poorly constrained, is to study white dwarfs for...
  • Publicación
    The Initial-Final Mass Relationship of White Dwarfs in Common Proper Motion Pairs and Open Clusters
    The initial-to-final mass relationship is the connection between the mass of a white dwarf and the mass of its progenitor in the main sequence. This function is...