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

  • Is the Core-cusp Problem a Matter of Perspective? Jeans Anisotropic Modeling against Numerical Simulations
    Mock member stars for 28 dwarf galaxies are constructed from the cosmological AURIGA simulation, which reflects the dynamical status of realistic stellar tracers. Axisymmetric Jeans Anisotropic Multi-Gaussian Expansion (JAM) modeling is applied to 6000 star particles for each system to recover the underlying matter distribution. The stellar or dark
    Wang, Wenting et al.

    Fecha de publicación:

    12
    2022
    Número de citas
    4
  • Lower-than-expected flare temperatures for TRAPPIST-1
    Aims: Stellar flares emit thermal and nonthermal radiation in the X-ray and ultraviolet (UV) regime. Although high energetic radiation from flares is a potential threat to exoplanet atmospheres and may lead to surface sterilization, it might also provide the extra energy for low-mass stars needed to trigger and sustain prebiotic chemistry. Despite
    Maas, A. J. et al.

    Fecha de publicación:

    12
    2022
    Número de citas
    4
  • Numerical simulations of catastrophic collisions of asteroids and fractions of impactor fragments included in remnants
    The Japanese spacecraft Hayabusa2 visited the asteroid Ryugu and conducted the detailed proximity observations. The observations show that Ryugu is a rubble-pile asteroid and it was formed through a catastrophic collision of a parent body (Watanabe et al. 2019). Ryugu's spectral features and the studies of orbital evolutions of asteroids suggest
    Sugiura, Keisuke et al.

    Fecha de publicación:

    12
    2022
    Número de citas
    0
  • Photometric Properties of Jupiter Trojans Detected by the Dark Energy Survey
    The Jupiter Trojans are a large group of asteroids that are coorbiting with Jupiter near its L4 and L5 Lagrange points. The study of Jupiter Trojans is crucial for testing different models of planet formation that are directly related to our understanding of solar system evolution. In this work, we select known Jupiter Trojans listed by the Minor
    Pan, Jiaming et al.

    Fecha de publicación:

    12
    2022
    Número de citas
    1