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

  • Do R Coronae Borealis stars evolve from white dwarf mergers?
    Phoenix spectra of C_2, CN and CO lines will provide oxygen isotopic abundance ratios (^16O/^17O/^18O) and CNO abundances for cool R Coronae Borealis (RCB) stars. The ratios, especially the ^16O/^18O ratio, will be used to test the two leading scenarios for RCB production. These observations were prompted by Clayton et al.'s striking discovery of
    Lambert, David L. et al.

    Fecha de publicación:

    2
    2008
    Número de citas
    0
  • Discovery of ultra-compact nuclear rings in three spiral galaxies
    Ring-shaped morphologies of nuclear star-forming regions within the central 40{-}200 pc of disk galaxies have been barely resolved so far in three composite Sy 2 nuclei, the Sy 2 Circinus galaxy and in three non-AGN galaxies. Such morphologies resemble those of the standard 1 kpc-size nuclear rings that lie in the inner Lindblad resonance regions
    Comerón, S. et al.

    Fecha de publicación:

    2
    2008
    Número de citas
    20
  • Discovery of a Wide Companion near the Deuterium-burning Mass Limit in the Upper Scorpius Association
    We present the discovery of a companion near the deuterium-burning mass limit located at a very wide distance, at an angular separation of 4.6''+/-0.1'' (projected distance of ~ 670 AU) from UScoCTIO 108, a brown dwarf of the very young Upper Scorpius association. Optical and near-infrared photometry and spectroscopy confirm the cool nature of both
    Béjar, V. J. S. et al.

    Fecha de publicación:

    2
    2008
    Número de citas
    85
  • Constraining the nature of high frequency peakers. II. Polarization properties
    Aims:The “bright” High Frequency Peakers (HFPs) sample is a mixture of blazars and intrinsically small and young radio sources. We investigate the polarimetric characteristics of 45 High Frequency Peakers, from the “bright” HFP sample, in order to have a deeper knowledge of the nature of each object, and to construct a sample made of genuine young
    Orienti, M. et al.

    Fecha de publicación:

    2
    2008
    Número de citas
    20
  • Bowen blend echo-tomography of low mass X-ray binaries
    We present simultaneous high time resolution (1-10 Hz) X-ray and optical observations of the persistent LMXBs Sco X-1 and V801 Ara( = 4U 1636-536). In the case of Sco X-1 we find that the Bowen/HeII emission lags the X-ray light-curves with a light travel time of ~11-16 s which is consistent with reprocessing in the donor star. We also present the
    Muñoz-Darias, T. et al.

    Fecha de publicación:

    2
    2008
    Número de citas
    7
  • ACO 1825 and AC 114 EROs photometry (Hempel+, 2008)
    New z-band (F850LP, denoted z850 hereafter) imaging was obtained with the ACS camera onboard HST in November 2004 (AC114) and July 2005 (Abell 1835). The 3.6, 4.5, 5.8, and 8.0{mu}m images were obtained using the Infrared Array Camera (IRAC), while the 24{mu}m images were obtained using the Multi-band Imaging Photometer for Spitzer (MIPS), both
    Hempel, A. et al.

    Fecha de publicación:

    2
    2008
    Número de citas
    0