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

  • Spitzer's Search for Proxima Centauri b Transits
    Proxima Centauri, the nearest star to the sun, hosts a habitable-zone planet (Anglada-Escude' et al. 2016 Nature 536, 437). Several teams have sought Proxima b's transits using ground-based photometry, and have reported tentative transit detections (Liu et al. 2018 AJ 155, 12; Blank et al. 2018 AJ 155, 228; others). Proxima, a modest-sized M-dwarf
    Harrington, Joseph et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    0
  • Spectral clustering tools applied to Ceres in preparation for the NASA OSIRIS-REx images of (101955) Bennu
    NASA's OSIRIS-REx mission is currently on its way to the asteroid (101955) Bennu. Bennu is a primitive asteroid, characterized by a dark surface composed mainly of carbon compounds, organic, and silicates altered by the presence of water. In addition, due to its proximity to the Earth, is classified as a potentially dangerous asteroid (PHA). Among
    Rizos, Juan et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    0
  • SMASHing the LMC: A Tidally Induced Warp in the Outer LMC and a Large-scale Reddening Map
    We present a study of the three-dimensional (3D) structure of the Large Magellanic Cloud (LMC) using ∼2.2 million red clump (RC) stars selected from the Survey of the MAgellanic Stellar History. To correct for line-of-sight dust extinction, the intrinsic RC color and magnitude and their radial dependence are carefully measured by using internal
    Choi, Yumi et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    92
  • SHEDDING LIGHT ON THE DARKEST GALAXIES: STRUCTURE AND SUBSTRUCTURES IN SEXTANS AND OTHER MILKY WAY DWARF SPHEROIDALS
    This thesis is focused on studying the structure and substructures in dwarf spheroidal galaxies (dSphs) satellites of the Milky Way (MW), mainly on the spatial distribution, but also on the internal kinematic and metallicity properties of their stellar component, from the analysis of large samples of individual stars. Due to the proximity of these
    Luis Cicuendez Salazar

    Fecha de publicación:

    10
    2018
  • Self-enrichment in globular clusters: the extreme He-rich populationof NGC 2808
    Almost several decades after the discovery of the first multiple populations in galactic globular clusters (GC), the debate on their formation is still extremely current and NGC 2808 remains one of the best benchmark to test any scenario for their origin and the evolution. In this work, we focus on the chemical composition of stars belonging to the
    Di Criscienzo, M. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    7
  • Raman, FT-IR spectroscopy and morphology of carbon dust from carbon arc in liquid benzene
    The carbon arc in liquid benzene produces carbon dust in addition to phenylacetyene and a number of other molecular products. The carbon dust was analyzed by Transmission Electron Microscopy (TEM), electron diffraction and Raman spectroscopy, revealing that it consists of a highly structured carbon black with high surface area. The carbon dust from
    García-Hernández, D. A. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    3