Tipo de publicación: Con árbitro

  • Publicación
    THE ORIENTATION OF LUGDUNUM CONUENARUM AND THE CELTIC FEASTS MARKING THE START OF THE SEASONS IN ANCIENT GAUL
    There is a long-lasting debate, started in the nineteenth century by d‟Arbois de Jubainville and Jullian, among others, regarding the pan-Celtic nature of the...
  • Publicación
    The Orientation of Pre-Romanesque Churches in the Iberian Peninsula
    The orientation of Christian churches is a distinctive feature of its architecture, repeating patterns from early Christian times that show a general tendency...
  • Publicación
    The orientation of WARPS in the Local Group.
    The three major spiral galaxies in the Local Group are known to be warped. The question is investigated of whether or not these three warps are aligned. Using...
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    The origin of accreted stellar halo populations in the Milky Way using APOGEE, Gaia, and the EAGLE simulations
    Recent work indicates that the nearby Galactic halo is dominated by the debris from a major accretion event. We confirm that result from an analysis of APOGEE...
  • Publicación
    The Origin of Asteroid 101955 (1999 RQ36)
    Near-Earth asteroid (NEA) 101955 (1999 RQ36; henceforth RQ36) is especially accessible to spacecraft and is the primary target of NASA's OSIRIS-REx sample...
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    The Origin of Asteroid 162173 (1999 JU3)
    Near-Earth asteroid (162173) 1999 JU3 (henceforth JU3) is a potentially hazardous asteroid and the target of the Japanese Aerospace Exploration Agency's...
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    The origin of bulges and discs in the CALIFA survey - I. Morphological evolution
    This series of papers aims at understanding the formation and evolution of non-barred disc galaxies. We use the new spectro-photometric decomposition code, C2D...
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    The origin of discs and spheroids in simulated galaxies
    The major morphological features of a galaxy are thought to be determined by the assembly history and net spin of its surrounding dark halo. In the simplest...
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    The origin of extended disc galaxies at z = 2
    Galaxy formation models typically assume that the size and rotation speed of galaxy discs are largely dictated by the mass, concentration and spin of their...