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

  • Multiple stellar populations in Magellanic Cloud clusters. II. Evidence also in the young NGC 1844?
    We used Hubble Space Telescope observations to study the young cluster NGC 1844 in the Large Magellanic Cloud (LMC). We estimated the fraction and the mass-ratio distribution of photometric binaries and report that the main sequence presents an intrinsic breadth which cannot be explained only in terms of photometric errors, and is unlikely because
    Milone, A. P. et al.

    Fecha de publicación:

    7
    2013
    Número de citas
    35
  • Kepler observations of very low-mass stars
    Observations of very low-mass stars with Kepler represent an excellent opportunity to search for planetary transits and to characterize optical photometric variability at the cool end of the stellar mass distribution. In this paper, we present low-resolution red optical spectra that allow us to identify 18 very low-mass stars that have Kepler light
    Martín, E. L. et al.

    Fecha de publicación:

    7
    2013
    Número de citas
    15
  • Hot bottom burning and s-process nucleosynthesis in massive AGB stars at the beginning of the thermally-pulsing phase
    We report the first spectroscopic identification of massive Galactic asymptotic giant branch (AGB) stars at the beginning of the thermal pulse (TP) phase. These stars are the most Li-rich massive AGBs found to date, super Li-rich AGBs with log ɛ (Li) ~ 3-4. The high Li overabundances are accompanied by weak or no s-process element (i.e. Rb and Zr)
    García-Hernández, D. A. et al.

    Fecha de publicación:

    7
    2013
    Número de citas
    72
  • HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-forming Galaxies
    We present measurements of the auto- and cross-frequency power spectra of the cosmic infrared background (CIB) at 250, 350, and 500 μm (1200, 860, and 600 GHz) from observations totaling ~70 deg2 made with the SPIRE instrument aboard the Herschel Space Observatory. We measure a fractional anisotropy δI/I = 14% ± 4%, detecting signatures arising
    Viero, M. P. et al.

    Fecha de publicación:

    7
    2013
    Número de citas
    156
  • Far infrared (terahertz) spectroscopy of a series of polycyclic aromatic hydrocarbons and application to structure interpretation of asphaltenes and related compounds
    A series of 33 different polycyclic aromatic hydrocarbons (PAHs) were studied by far infrared spectroscopy (terahertz spectroscopy) in the spectral range comprised between 600 and 50 cm(-1). In addition to common PAHs like naphthalene, anthracene, phenanthrene, fluoranthene, picene, pyrene, benzo[α]pyrene, and perylene, also quite unusual PAHs were
    Manchado, A. et al.

    Fecha de publicación:

    7
    2013
  • Evolution of the Fundamental Plane for early-type galaxies up to z = 1.2
    We studied the evolution of the Fundamental Plane in B- and g-bands, for two samples of early-type galaxies at 0.2 z 0.35 and 0.35 z 1.2. We found a difference in the intercept that can be interpreted as galaxies at z > ~0.7 being 0.68 and 0.52 mag brighter in the B- and g-band respectively, than their local counterparts. From the study of the
    Fernández-Lorenzo, M. et al.

    Fecha de publicación:

    7
    2013
    Número de citas
    0