Tipo de publicación: Sin árbitro

  • Publicación
    Fullerenes as carriers of extinction, diffuse interstellar bands and anomalous microwave emission
    According to semiempirical models, photoabsorption by fullerenes (single and multishell) could explain the shape, width and peak energy of the most prominent...
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    Fully Adaptive Bayesian Algorithm for Data Analysis. FABADA
    The discovery potential from astronomical and other data is limited by their noise. We introduce a novel non-parametric noise reduction technique based on...
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    Fully cosmological virtual galaxies from MASCLET
    We present the study of the most massive galaxies (M^{*}>10^{11} {M}_{&sun;}) found in a cosmological simulation performed with MASCLET (Mesh Adaptative Scheme...
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    Fundamental parameters of low mass X-ray binaries II: X-ray persistent systems
    The determination of fundamental parameters in X-ray luminous (persistent) X-ray binaries has been classically hampered by the large optical luminosity of the...
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    Fundamental parameters of stars (Allende Prieto+, 1999)
    The Hipparcos mission has made it possible to constrain the positions of nearby field stars in the colour-magnitude diagram with very high accuracy. These...
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    Fundamental Physics with Brown Dwarfs: The Mass-Radius Relation
    The lowest-mass stars, brown dwarfs and giant exoplanets span a minimum in the mass-radius relationship that probes the fundamental physics of extreme states of...
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    Fundamental properties of high mass X-ray binaries
    High mass X-ray binaries (HMXBs) are important laboratories where to study the characteristics of the accretion processes and the nature of compact objects. For...
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    Fundamental Stellar Parameters Derived From High-Resolution High Signal-To-Noise Spectra of Stars Within 15pc of the Sun
    High-resolution spectra of a sample of all known stars more luminous than MV=+6.5 and closer than 15 parsecs are being analyzed spectroscopically in order to...
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    Further Chandra observations of SAX J1747.0-2853 and the region around Sgr A*
    On 20-21 October 2005, the remaining six Chandra/HRC-I observations (as mentioned in ATEL #637) were performed as part of the XMM-Newton/ Chandra monitoring...