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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  • Modeling Close Binary Systems Within Planetary Nebulae
    We present here binary modeling for the close binary central star of the planetary nebula Hf 2-2. While binary models for 26 close binary star systems within a planetary nebula exist, this number is far too low to perform a significant statistical analysis. In order to work towards increasing this number, and thus improving the statistical results
    Blanton, Lilly et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    0
  • Modeling Binary Systems Containing the Hot White Dwarfs WD1136+667 and Gaia-DR2-1350
    In this study, we look specifically at binary white dwarfs where the companion is a main sequence star. In particular, we look at very hot white dwarfs, many of which demonstrate the "hydrogen problem" in which modeling of their hydrogen absorption features, and optical features in general, do not appear to give accurate temperatures. The two
    Wood, Hunter et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    0
  • MANCHA3D Code: Multipurpose Advanced Nonideal MHD Code for High-Resolution Simulations in Astrophysics
    The MANCHA3D code is a versatile tool for numerical simulations of magnetohydrodynamic (MHD) processes in solar/stellar atmospheres. The code includes nonideal physics derived from plasma partial ionization, a realistic equation of state and radiative transfer, which allows performing high-quality realistic simulations of magnetoconvection, as well
    Modestov, M. et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    10
  • JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs
    We present JWST images of the well-known planetary nebula NGC 6720 (the Ring Nebula), covering wavelengths from 1.6 to 25 $\, \mu$m. The bright shell is strongly fragmented with some 20 000 dense globules, bright in H 2, with a characteristic diameter of 0.2 arcsec and density n H ~ 10 5-10 6 cm -3. The shell contains a narrow ring of polycyclic
    Wesson, R. et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    16
  • Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?
    We present a comprehensive analysis of the Hubble Space Telescope observations of the atmosphere of WASP-121 b, an ultra-hot Jupiter. After reducing the transit, eclipse, and phase-curve observations with a uniform methodology and addressing the biases from instrument systematics, sophisticated atmospheric retrievals are used to extract robust
    Changeat, Q. et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    27
  • INCIDENCE AND ENERGETICS OF AGN WINDS IN THE LOCAL UNIVERSE
    El crecimiento de las galaxias masivas está estrictamente relacionado con la acreción de materia en su centro, donde residen los Agujeros Negros Supermasivos (SMBH). Los Núcleos Activos de Galaxias (AGN) exhiben caminos evolutivos in- terdependientes con sus galaxias anfitrionas a través de un intercambio continuo de energía y materia mediante
    Giovanna Speranza

    Fecha de publicación:

    2
    2024