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

  • A comparative study of resistivity models for simulations of magnetic reconnection in the solar atmosphere. II. Plasmoid formation

    Context. Plasmoid-mediated reconnection plays a fundamental role in different solar atmospheric phenomena. Numerical reproduction of this process is therefore essential for developing robust solar models. Aims: Our goal is to assess plasmoid-mediated reconnection across various numerical resistivity models in order to investigate how plasmoid

    Færder, Ø. H. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Accretion-induced flickering variability among symbiotic stars from space photometry with NASA TESS

    Context. Symbiotic binaries exhibit a wide range of photometric variability across different timescales. These changes can be attributed to factors such as orbital motion, intrinsic variability of the individual components, or interactions between the two stars. In the range from minutes to hours, a variability induced by accretion processes that

    Merc, J. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Comparing Observed with Simulated Solar-disk-center Scattering Polarization in the Sr I 4607 Å Line

    Solar magnetic fields alter scattering polarization in spectral lines like Sr I at 4607 Å via the Hanle effect, making it a potential diagnostic for small-scale, mixed-polarity photospheric magnetic fields. Recently, observational evidence for scattering polarization in the Sr I 4607 Å line at the solar disk center was found. Here, we investigate

    Zeuner, Franziska et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Evidence for transit-timing variations of the 11 Myr exoplanet TOI-1227 b

    TOI-1227 b is an 11 Myr old validated transiting planet in the middle of its contraction phase, with a current radius of 0.85 Rj. It orbits a low-mass pre-main sequence star (0.170 M⊙, 0.56 R⊙) every 27.4 days. The magnetic activity of its young host star induces radial velocity jitter and prevents good measurements of the planetary mass. We

    Almenara, J. M. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Magnetic field amplification and structure formation by the Rayleigh-Taylor instability (Corrigendum)
    Popescu Braileanu, B. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • NGDEEP Epoch 1: Spatially Resolved Hα Observations of Disk and Bulge Growth in Star-forming Galaxies at z ∼ 0.6–2.2 from JWST NIRISS Slitless Spectroscopy

    We study the Hα equivalent width (EW(Hα)) maps of 19 galaxies at 0.6 < z < 2.2 in the Hubble Ultra Deep Field using NIRISS slitless spectroscopy as part of the Next Generation Deep Extragalactic Exploratory Public Survey. Our galaxies mostly lie on the star formation main sequence with stellar masses between 109 and 1011 M ⊙, characterized as

    Shen, Lu et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0