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

  • S-process nucleosynthesis in AGB stars with the full spectrum of turbulence scheme for convection.
    The chemical evolution of asymptotic giant branch (AGB) stars models depends greatly on the input physics (e.g. convective model, mass loss recipe). Variations of hot bottom burning (HBB) strength, or third dredge-up (TDU) efficiency are among the main consequences of adopting different input physics in the AGB models. The ATON evolutionary code
    Yagüe, A. et al.

    Fecha de publicación:

    7
    2016
    Número de citas
    0
  • Rb and Zr abundances in massive Galactic AGB stars revisited
    We report new abundances of Rb and Zr in a sample of massive Galactic asymptotic giant branch (AGB) stars that were previously studied with hydrostatic models by using more realistic dynamical model atmospheres. We use a modified version of the spectral synthesis code Turbospectrum, and consider the presence of a circumstellar envelope and a radial
    Pérez-Mesa, V. et al.

    Fecha de publicación:

    7
    2016
    Número de citas
    0
  • On the Magnetism and Dynamics of Prominence Legs Hosting Tornadoes
    Solar tornadoes are dark vertical filamentary structures observed in the extreme ultraviolet associated with prominence legs and filament barbs. Their true nature and relationship to prominences requires an understanding of their magnetic structure and dynamic properties. Recently, a controversy has arisen: is the magnetic field organized forming
    Martínez González, M. J. et al.

    Fecha de publicación:

    7
    2016
    Número de citas
    17
  • On the formation of molecules and solid-state compounds from the AGB to the PN phases
    During the asymptoyic giant branch (AGB) phase, different elements are dredge- up to the stellar surface depending on progenitor mass and metallicity. When the mass loss increases at the end of the AGB, a circumstellar dust shell is formed, where different (C-rich or O-rich) molecules and solid-state compounds are formed. These are further
    García-Hernández, D. A. et al.

    Fecha de publicación:

    7
    2016
    Número de citas
    0
  • Numerical simulations of magnetic Kelvin-Helmholtz instability at a twisted solar flux tube
    The paper aims to study the response of a solar small-scale and weak magnetic flux tube to photospheric twisting motions. We numerically solve three-dimensional ideal magnetohydrodynamic equations to describe the evolution of the perturbation within the initially static flux tube, excited by twists in the azimuthal component of the velocity. These
    Murawski, K. et al.

    Fecha de publicación:

    7
    2016
    Número de citas
    8
  • No sign (yet) of intergalactic globular clusters in the Local Group
    We present Gemini Multi-Object Spectrograph (GMOS) imaging of 12 candidate intergalactic globular clusters (IGCs) in the Local Group, identified in a recent survey of the Sloan Digital Sky Survey (SDSS) footprint by di Tullio Zinn & Zinn. Our image quality is sufficiently high, at ˜0.4-0.7 arcsec, that we are able to unambiguously classify all 12
    Mackey, A. D. et al.

    Fecha de publicación:

    7
    2016
    Número de citas
    9