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

  • Spirals and rings: how do they form? What are their structure and properties?
    Not Available
    Athanassoula, L. et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    0
  • Spatial variations in the star formation history of the Large Magellanic Cloud
    Based on the quantitative analysis of a set of wide-field color—magnitude diagrams reaching the old main sequence-turnoffs, we present new LMC star-formation histories, and their variation with galactocentric distance. Some coherent features are found, together with systematic variations of the star-formation history among the three fields analyzed
    Gallart, Carme et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    3
  • SPACE: the spectroscopic all-sky cosmic explorer
    We describe the scientific motivations, the mission concept and the instrumentation of SPACE, a class-M mission proposed for concept study at the first call of the ESA Cosmic-Vision 2015-2025 planning cycle. SPACE aims to produce the largest three-dimensional evolutionary map of the Universe over the past 10 billion years by taking near-IR spectra
    Cimatti, A. et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    70
  • Robust Determination of the Major Merger Fraction at z = 0.6 in the Groth Strip
    We measure the fraction of galaxies undergoing disk-disk major mergers (f mph m ) at intermediate redshifts (0.35
    López-Sanjuan, Carlos et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    38
  • Refined Orbital Solution and Quiescent Variability in the Black Hole Transient GS 1354-64 (= BW Cir)
    In Casares et al. we presented the first radial velocity curve of the companion star to BW Cir which demonstrates the presence of a black hole in this historical X-ray transient. But these data were affected by aliasing and two possible periods at 2.5445 days and 2.5635 days were equally possible. Here we present new spectroscopic data that enable
    Casares, J. et al.

    Fecha de publicación:

    3
    2009
    Número de citas
    73