Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Angular Size Test on the Expansion of the Universe
    Assuming the standard cosmological model to be correct, the average linear size of the galaxies with the same luminosity is six times smaller at z = 3.2 than at z = 0; and their average angular size for a given luminosity is approximately proportional to z-1. Neither the hypothesis that galaxies which formed earlier have much higher densities nor
    López-Corredoira, Martín

    Fecha de publicación:

    1
    2010
    Número de citas
    23
  • AINUR (Atlas of Images of Nuclear Rings)
    Nuclear rings are in most cases thought to be by-products of gas shock-focusing at Inner Lindblad Resonances (ILRs). AINUR (Atlas of Images of NUclear Rings) is an Atlas which includes images and metric measurements of all 109 known nuclear rings. This Atlas has been produced by checking and processing Hubble Space Telescope archive data from a
    Comerón, S. et al.

    Fecha de publicación:

    1
    2010
    Número de citas
    0
  • A Two Micron All Sky Survey View of the Sagittarius Dwarf Galaxy. VI. s-Process and Titanium Abundance Variations Along the Sagittarius Stream
    We present high-resolution spectroscopic measurements of the abundances of the α element titanium (Ti) and s-process elements yttrium (Y) and lanthanum (La) for 59 candidate M giant members of the Sagittarius (Sgr) dwarf spheroidal (dSph) + tidal tail system pre-selected on the basis of position and radial velocity (RV). As expected, the majority
    Chou, Mei-Yin et al.

    Fecha de publicación:

    1
    2010
    Número de citas
    60
  • What Can the Radial Surface Brightness Profiles of Galaxy Discs Tell Us About Their Evolution?
    Deriving the azimuthally averaged radial surface brightness profile of a galaxy is a schematic way of presenting the light and then the mass structure of disc galaxies. In this overview we will dwell on the outer discs, as it has become possible, with modern data to explore the light profile out to ever increasing galactocentric radii. We find that
    Beckman, John E. et al.

    Fecha de publicación:

    0
    2010
    Número de citas
    0
  • Weak Flares on M-Dwarfs
    We have investigated the physics of flares in M-dwarfs by means of optical/X-ray observations and modeling. The great efficiency of current optical spectrographs and detectors has allowed us to detect and analyze a great number of non white-light flares with intermediate spectral resolution and high temporal resolution. Although this kind of flares
    Crespo-Chacón, I. et al.

    Fecha de publicación:

    0
    2010
    Número de citas
    0
  • UV intensity distributions of the quiet Sun observed with Sunrise
    High resolution solar images in the near UV have been obtained with the Solar UV Filtergraph (SUFI) onboard the Sunrise balloon borne observatory, amongst others in wavelength regions not accessible from the ground. We present intensity distributions of the quiet Sun at different heliocentric angles, from disk center to the solar limb. These
    Hirzberger, Johann et al.

    Fecha de publicación:

    0
    2010
    Número de citas
    0