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..

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  • Abundance ratios in dwarf elliptical galaxies
    We determine abundance ratios of 37 dwarf ellipticals (dEs) in the nearby Virgo cluster. This sample is representative of the early-type population of galaxies in the absolute magnitude range -19.0 Mr -16.0. We analyse their absorption line-strength indices by means of index-index diagrams and scaling relations and use the stellar population
    Şen, Ş. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    13
  • Abundance ratios & ages of stellar populations in HARPS-GTO sample
    In this work we present chemical abundances of heavy elements (Z>28) for a homogeneous sample of 1059 stars from HARPS planet search program. We also derive ages using parallaxes from Hipparcos and Gaia DR1 to compare the results. We study the [X/Fe] ratios for different populations and compare them with models of Galactic chemical evolution. We
    Delgado Mena, E. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    7
  • A view of the H-band light-element chemical patterns in globular clusters under the AGB self-enrichment scenario
    We discuss the self-enrichment scenario by asymptotic giant branch (AGB) stars for the formation of multiple populations in globular clusters (GCs) by analysing data set of giant stars observed in nine Galactic GCs, covering a wide range of metallicities and for which the simultaneous measurements of C, N, O, Mg, Al, and Si are available. To this
    Dell'Agli, F. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    28
  • A photometric study of globular clusters observed by the APOGEE survey
    In this paper, we describe the photometric and spectroscopic properties of multiple populations in seven northern globular clusters. In this study, we employ precise ground-based photometry from the private collection of Stetson, space photometry from the Hubble Space Telescope (HST), literature abundances of Na and O, and Apache Point Observatory
    Mészáros, Sz. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    6
  • A deep narrowband survey for planetary nebulae at the outskirts of M 33
    Context. Planetary nebulae (PNe) are excellent tracers of stellar populations with low surface brightness, and therefore provide a powerful method to detect and explore the rich system of substructures discovered around the main spiral galaxies of the local group. Aim. We searched the outskirts of the local group spiral galaxy M 33 (the Triangulum)
    Galera-Rosillo, R. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    6
  • SPECTROSCOPIC AND PHOTOMETRIC CHARACTERIZATION OF PRIMITIVE ASTEROID COLLISIONAL FAMILIES
    The study of near-Earth asteroids (NEAs) is very important, due to three main reasons. First, they pose an impact risk for Earth, and damage produced by a possible collision will depend on the speed of the impact, the size of the object, and its composition. Second, given their proximity, they are easy access targets for the visit of space missions
    David Morate González

    Fecha de publicación:

    4
    2018