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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  • The Double-Barred Galaxy NGC 357: Kinematics and Stellar Populations
    We have carried out a complete analysis of the kinematics and the stellar populations of the double-barred S0 galaxy NGC 357. We have measured suitable absorption line strength indices on very high quality spectra. With the aid of stellar population models we have obtained the relative ages and metallicities for the different components to
    de Lorenzo-Cáceres, A. et al.

    Fecha de publicación:

    12
    2007
    Número de citas
    0
  • The Dwarf Galaxy Leo A: A Survivor From the Epoch of Reionization
    We present the results of a program to derive the complete star-formation history of the Local Group dwarf irregular galaxy Leo A (DDO 69). Leo A is a low-luminosity (Mv = -11.7), very gas-rich (M(HI)/LB = 1.6) galaxy. Our analysis is based on color-magnitude diagrams derived from deep HST/ACS imaging; the CMDs reach well below the oldest main
    Cole, Andrew A. et al.

    Fecha de publicación:

    12
    2006
    Número de citas
    0
  • The Dwarf Spheroidal Galaxies Around the Milky Way
    We review the progress of ESO/WFI Imaging and VLT/FLAMES spectroscopy of large numbers of individual stars in nearby dwarf spheroidal galaxies by the Dwarf Abundances and Radial-velocities Team (DART). These observations have allowed us to show that neither the kinematics nor the abundance nor the spatial distributions are easy to explain in a
    Tolstoy, E. et al.

    Fecha de publicación:

    12
    2007
    Número de citas
    0
  • The Dynamical Evolution of the Circumstellar Gas around Low- and Intermediate-Mass Stars. II. The Planetary Nebula Formation
    We have studied the effect of the mass of the central star (CS) on the gas evolution during the planetary nebula (PN) phase. We have performed numerical simulations of PN formation using CS tracks for six stellar core masses corresponding to initial masses from 1 to 5 Msolar. The gas structure resulting from the previous asymptotic giant branch
    Villaver, Eva et al.

    Fecha de publicación:

    12
    2002
    Número de citas
    119
  • The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme
    We present results from a subset of simulations from the `Evolution and Assembly of GaLaxies and their Environments' (EAGLE) suite in which the formulation of the hydrodynamics scheme is varied. We compare simulations that use the same subgrid models without recalibration of the parameters but employing the standard GADGET flavour of smoothed
    Schaller, M. et al.

    Fecha de publicación:

    12
    2015
    Número de citas
    205
  • The Earth as an object of astrophysical interest in the search for extrasolar planets
    The potential discovery of Earth-like planets around other stars will need, apart from a sophisticated technological development, the design of techniques for identifying the most representative parameters of their atmospheres and surfaces. The search for life will constitutes the holy grail of this search. However, for many decades the
    Vázquez, M. et al.

    Fecha de publicación:

    12
    2006
    Número de citas
    1